Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6.

The existence of massive (1011 solar masses) elliptical galaxies by redshift z ≈ 4 (refs 1, 2, 3; when the Universe was 1.5 billion years old) necessitates the presence of galaxies with star-formation rates exceeding 100 solar masses per year at z > 6 (corresponding to an age of the Universe of less than 1 billion years). Surveys have discovered hundreds of galaxies at these early cosmic epochs, but their star-formation rates are more than an order of magnitude lower. The only known galaxies with very high star-formation rates at z > 6 are, with one exception, the host galaxies of quasars, but these galaxies also host accreting supermassive (more than 109 solar masses) black holes, which probably affect the properties of the galaxies. Here we report observations of an emission line of singly ionized carbon ([C ii] at a wavelength of 158 micrometres) in four galaxies at z > 6 that are companions of quasars, with velocity offsets of less than 600 kilometres per second and linear offsets of less than 100 kiloparsecs. The discovery of these four galaxies was serendipitous; they are close to their companion quasars and appear bright in the far-infrared. On the basis of the [C ii] measurements, we estimate star-formation rates in the companions of more than 100 solar masses per year. These sources are similar to the host galaxies of the quasars in [C ii] brightness, linewidth and implied dynamical mass, but do not show evidence for accreting supermassive black holes. Similar systems have previously been found at lower redshift. We find such close companions in four out of the twenty-five z > 6 quasars surveyed, a fraction that needs to be accounted for in simulations. If they are representative of the bright end of the [C ii] luminosity function, then they can account for the population of massive elliptical galaxies at z ≈ 4 in terms of the density of cosmic space.

Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.

The rest-frame ultraviolet properties of galaxies during the first three billion years of cosmic time (redshift z > 4) indicate a rapid evolution in the dust obscuration of such galaxies. This evolution implies a change in the average properties of the interstellar medium, but the measurements are systematically uncertain owing to untested assumptions and the inability to detect heavily obscured regions of the galaxies. Previous attempts to measure the interstellar medium directly in normal galaxies at these redshifts have failed for a number of reasons, with two notable exceptions. Here we report measurements of the forbidden C ii emission (that is, [C II]) from gas, and the far-infrared emission from dust, in nine typical star-forming galaxies about one billion years after the Big Bang (z ≈ 5-6). We find that these galaxies have thermal emission that is less than 1/12 that of similar systems about two billion years later, and enhanced [C II] emission relative to the far-infrared continuum, confirming a strong evolution in the properties of the interstellar medium in the early Universe. The gas is distributed over scales of one to eight kiloparsecs, and shows diverse dynamics within the sample. These results are consistent with early galaxies having significantly less dust than typical galaxies seen at z < 3 and being comparable in dust content to local low-metallicity systems.

The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts.

Most of the baryons in galaxy clusters reside between the galaxies in a hot, tenuous gas. The densest gas in their centres should cool and accrete onto giant central galaxies at rates of 10-1,000 solar masses per year. No viable repository for this gas, such as clouds or new stars, has been found. New X-ray observations, however, have revealed far less cooling below X-ray temperatures than expected, altering the previously accepted picture of cooling flows. As a result, most of the gas must be heated to and maintained at temperatures above approximately 2 keV (ref. 3). The most promising heating mechanism is powerful radio jets emanating from supermassive black holes in the central galaxies of clusters. Here we report the discovery of giant cavities and shock fronts in a distant (z = 0.22) cluster caused by an interaction between a radio source and the hot gas surrounding it. The energy involved is approximately 6 x 10(61) erg, the most powerful radio outburst known. This is enough energy to quench a cooling flow for several Gyr, and to provide approximately 1/3 keV per particle of heat to the surrounding cluster.

The essential signature of a massive starburst in a distant quasar.

Observations of carbon monoxide emission in high-redshift (zeta > 2) galaxies indicate the presence of large amounts of molecular gas. Many of these galaxies contain an active galactic nucleus powered by accretion of gas onto a supermassive black hole, and a key question is whether their extremely high infrared luminosities result from the active galactic nucleus, from bursts of massive star formation (associated with the molecular gas), or both. In the Milky Way, high-mass stars form in the dense cores of interstellar molecular clouds, where gas densities are n(H2) > 10(5) cm(-3) (refs 1, 2). Recent surveys show that virtually all galactic sites of high-mass star formation have similarly high densities. The bulk of the cloud material traced by CO observations, however, is at a much lower density. For galaxies in the local Universe, the HCN molecule is an effective tracer of high-density molecular gas. Here we report observations of HCN emission from the infrared-luminous 'Cloverleaf' quasar (at a redshift zeta = 2.5579). The HCN line luminosity indicates the presence of 10 billion solar masses of very dense gas, an essential feature of an immense starburst, which contributes, together with the active galactic nucleus it harbours, to its high infrared luminosity.

Structure of recombinant human renin, a target for cardiovascular-active drugs, at 2.5 A resolution.

The x-ray crystal structure of recombinant human renin has been determined. Molecular dynamics techniques that included crystallographic data as a restraint were used to improve an initial model based on porcine pepsinogen. The present agreement factor for data from 8.0 to 2.5 angstroms (A) is 0.236. Some of the surface loops are poorly determined, and these disordered regions border a 30 A wide solvent channel. Comparison of renin with other aspartyl proteinases shows that, although the structural cores and active sites are highly conserved, surface residues, some of which are critical for specificity, vary greatly (up to 10A). Knowledge of the actual structure, as opposed to the use of models based on related enzymes, should facilitate the design of renin inhibitors.

Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.

The largest galaxies in the universe reside in galaxy clusters. Using sensitive observations of carbon monoxide, we show that the Spiderweb galaxy-a massive galaxy in a distant protocluster-is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched intergalactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift.

Characterization of recombinant human prorenin and renin.

A cell line that secretes substantial quantities of recombinant human prorenin was prepared by transfecting Chinese hamster ovary cells with a gene encoding preprorenin. The prorenin was purified to homogeneity and was found to have a single amino terminus, reflecting cleavage after a typical 23 amino acid signal sequence. The purified inactive prorenin was not a substrate for active renin and was not capable of self-activation. Prorenin could be converted to renin by addition of exogenous protease, and deglycosylation of the prorenin did not alter the sensitivity to protease activation. The enzymatic activity of deglycosylated renin was kinetically identical to that of the native protein. Multimilligram quantities of recombinant human renin and prorenin were purified, providing suitable material for studies directed toward greater understanding of the function of these proteins and for structural studies such as x-ray diffraction for use in design of renin inhibitors.

Infusion of recombinant human prorenin into rhesus monkeys. Effects on hemodynamics, renin-angiotensin-aldosterone axis and plasma testosterone.

Prorenin, the biosynthetic precursor of active renin, is present in high concentrations in the kidney and reproductive organs. We have proposed that prorenin may be the vehicle of local renin systems, separating the functions of circulating and tissue renin. In the present study, we investigated the effect of increasing plasma prorenin 3- to 4-fold by infusing recombinant prorenin, 400 ng/min for 40 min, into male rhesus monkeys. The prorenin was first warmed to 37 degrees C to reduce the endogenous renin activity to a minimum. The study included a 20 min baseline and a 40 min recovery period. Plasma prorenin increased from 72 +/- 14 ng/mL/h to a maximum of 246 +/- 18 ng/mL/h during the infusion (P less than .001) and fell to 169 +/- 23 ng/mL/h 40 min after the infusion was stopped. Active renin did not change significantly. Plasma aldosterone increased slightly during the prorenin infusion (by 13%) and returned to baseline during the recovery period (P less than .05 compared to the infusion period). Plasma testosterone fell significantly from 1.9 +/- 0.1 ng/mL to 1.6 +/- 0.1 ng/mL during the infusion and further to 1.4 +/- 0.1 ng/mL during the post-infusion period (P less than .05). Blood pressure fell slightly but not significantly. Heart rate, glomerular filtration rate and renal blood flow, as well as urine flow and urine sodium and potassium excretion showed no significant change. These results demonstrate that human recombinant prorenin is not converted to active renin in the circulation of rhesus monkeys.(ABSTRACT TRUNCATED AT 250 WORDS)

Constraints on changes in fundamental constants from a cosmologically distant OH absorber or emitter.

We have detected the four 18 cm OH lines from the z approximaetely 0.765 gravitational lens toward PMN J0134-0931. The 1612 and 1720 MHz lines are in conjugate absorption and emission, providing a laboratory to test the evolution of fundamental constants over a large lookback time. We compare the HI and OH main line absorption redshifts of the different components in the z approximately 0.765 absorber and the z approximately 0.685 lens toward B0218 + 357 to place stringent constraints on changes in F triple-bond g(p)[alpha(2)/mu](1.57). We obtain [DeltaF/F] = (0.44 +/- 0.36(stat) +/- 1.0(sys)t) x 10(-5), consistent with no evolution over the redshift range 0 < z < or = 0.7. The measurements have a 2sigma sensitivity of [Deltaalpha/alpha] < 6.7 x 10(-6) or [Deltamu/mu] < 1.4 x 10(-5) to fractional changes in alpha and mu over a period of approximately 6.5 G yr, half the age of the Universe. These are among the most sensitive constraints on changes in mu.

Hypothalamic sodium-transport inhibitor is a high-affinity reversible inhibitor of Na+-K+-ATPase.

Bovine hypothalamus contains a stable, low molecular weight substance with ouabain-like properties. To further study its mechanism of action and potential physiological importance we examined its effects on purified Na+-K+-ATPase in a kinetic coupled-enzyme assay. Under optimal conditions up to 95% of Na+-K+-ATPase activity could be inhibited by the factor. Mg2+ is required for maximal inhibitory activity, but ligand requirements for optimal activity are otherwise distinct from those of both ouabain and vanadate. Inhibition is reversed by high concentrations of sodium chloride plus EDTA. Kinetic analysis yielded a Ki = 1.4 nM. The hypothalamic factor is a high-affinity reversible inhibitor of Na+-K+-ATPase, being at least as potent as the cardiac glycoside ouabain and may be a circulating inhibitor of sodium transport, which appears to be associated with experimental volume-expanded hypertension and human essential hypertension.

A massive reservoir of low-excitation molecular gas at high redshift.

Molecular hydrogen (H2) is an important component of galaxies because it fuels star formation and the accretion of gas onto active galactic nuclei (AGN), the two processes that can generate the large infrared luminosities of gas-rich galaxies. Observations of spectral-line emission from the tracer molecule carbon monoxide (CO) are used to probe the properties of this gas. But the lines that have been studied in the local Universe-mostly the lower rotational transitions of J = 1 --> 0 and J = 2 --> 1-have hitherto been unobservable in high-redshift galaxies. Instead, higher transitions have been used, although the densities and temperatures required to excite these higher transitions may not be reached by much of the gas. As a result, past observations may have underestimated the total amount of molecular gas by a substantial amount. Here we report the discovery of large amounts of low-excitation molecular gas around the infrared-luminous quasar APM08279+5255 at redshift z = 3.91, using the two lowest excitation lines of 12 CO (J = 1 --> 0 and J = 2 --> 1). The maps confirm the presence of hot and dense gas near the nucleus, and reveal an extended reservoir of molecular gas with low excitation that is 10 to 100 times more massive than the gas traced by the higher-excitation observations. This raises the possibility that significant amounts of low-excitation molecular gas may exist in the environments of high-redshift (z > 3) galaxies.

The nuclear jet and counterjet region of the radio galaxy Cygnus A.

Very-long-baseline interferometry images of the nuclear region of the radio galaxy Cygnus A reveal a pronounced "core" and a knotty jet and counterjet. The knots are moving away from the core at apparent speeds which are subluminal for h = 1 [h = H0/100 km.s-1.Mpc-1;1 parsec (pc) = 3.09 x 10(16)m] and about c for h = 0.5. The jet is aligned with the outer, kiloparsec-scale jet to within 2 degrees. The counterjet has a total flux density at 5 GHz of about one-fifth of that of the jet. In the context of the twin relativistic jet model for active galactic nuclei, the jet in Cygnus A is oriented at an angle to our line of sight of 35-80 degrees and 55-85 degrees, and the intrinsic velocity of the jet fluid is 0.4-0.6c and 0.6-1c for h = 1 and h = 0.5, respectively.

The amino acid sequence of a fluorescein-labeled peptide from the active site of (Na,K)-ATPase.

(Na,K)-ATPase in an active-transport protein that couples the energy obtained from the hydrolysis of ATP to the transport of Na+ and K+ across animal cell membranes. In order to investigate the enzymatic mechanism of this activity, a peptide derived from the ATP-binding site of (Na,K)-ATPase has been purified and its amino acid sequence has been determined. The peptide was identified by the covalent incorporation of a fluorescent probe, fluorescein 5'-isothiocyanate, into the active site before trypsin digestion of the protein. The labeling of (Na,K)-ATPase by fluorescein 5'-isothiocyanate was associated with the irreversible inhibition of enzymatic activity, and both the labeling of the tryptic peptide and inhibition of activity were prevented when the reaction was performed in the presence of ATP. An apparent KD of 5.7 microM was calculated when the reaction between (Na,K)-ATPase and fluorescein 5'-isothiocyanate was performed under pseudo first-order conditions. The amino acid sequence of the active-site peptide, His-Leu-Leu-Val-Met-Lys-Gly-Ala-Pro-Glu-Arg, is similar to the sequence of a fluorescein-labeled peptide derived from the active site of the sarcoplasmic reticulum Ca2+-transport ATPase (Mitchinson, C., Wilderspin, A. F., Trinaman, B. J., and Green, N. M. (1982) FEBS Lett. 146, 87-92).

Hypothalamic factor inhibits the (Na,K)ATPase from the extracellular surface. Mechanism of inhibition.

We have characterized the effect of a stable small molecule isolated from bovine hypothalamus (Haupert, G. T., and Sancho, J. M. (1979) Proc. Natl. Acad. Sci. 76, 4658-4660) on mammalian (Na,K)ATPase. This hypothalamus-derived inhibitory factor, HIF, has been shown to inhibit ATPase activity of purified dog kidney enzyme reversibly with high affinity (Haupert, G. T., Carilli, C. T., and Cantley, L. C. (1984) Am. J. Physiol. 247, F919-F924). In this report it is shown that HIF inhibits the ouabain sensitive component of 86Rb+ uptake into human red blood cells. HIF also inhibited (Na,K)ATPase activity of unsealed red cell membranes but not that of sealed inside-out vesicles, indicating that HIF is impermeant to red cell membranes and inhibits the (Na,K)ATPase from the extracellular side. In unsealed human red cell membranes, concentrations of HIF which caused 70% inhibition of the (Na,K)ATPase did not inhibit ATP hydrolysis by plasma membrane (Ca2+)ATPase or (Mg2+)ATPase. However, at a similar concentration, HIF was shown to inhibit rabbit muscle sarcoplasmic reticulum (Ca2+)ATPase. HIF also inhibited p-nitrophenylphosphatase activity of unmodified or fluorescein-5'-iso-thiocyanate labeled dog kidney (Na,K)ATPase. As judged by fluorescein fluorescence of the modified enzyme, HIF stabilized the low fluorescent "E2" conformation of the enzyme similar to that stabilized by ouabain. However, unlike ouabain, HIF blocked covalent phosphorylation of dog kidney (Na,K)ATPase by inorganic phosphate. These studies show that HIF is an inhibitor of (Na,K)ATPase which acts from the extracellular side of the membrane by a mechanism similar to but not identical to that of cardiac glycosides.

The active site structure of Na+- and K+-stimulated ATPase. Location of a specific fluorescein isothiocyanate reactive site.

Fluorescein 5'-isothiocyanate (FITC) has been shown to specifically inactivate the Na+- and K+-stimulated adenosine triphosphatase ((Na,K)-ATPase) at low concentrations (Karlish, S. J. D. (1979) Na+,K+ATPase Structure and Kinetics 115-128). The site of modification of purified dog kidney (Na,K)-ATPase by FITC has been investigated by enzymatic cleavage and fluorescence resonance energy transfer. The binding of FITC, which occurs at a stoichiometry of approximately one site per ATP binding site, causes an ATP-protectable inactivation of ATPase activity suggesting that it is reacting at the ATP hydrolysis site. The FITC reaction site apparently is located near the center of the COOH-terminal 77,000-dalton peptide fragment obtained by chymotryptic cleavage of the alpha subunit. Addition of ouabain to the native enzyme in the presence of chymotrypsin enhances cleavage at this site and releases the fluorescein moiety from the membrane. It is further shown that the distance from the FITC reaction site to the ouabain binding site, as judged by fluorescence resonance energy transfer from anthroyl ouabain to FITC, is approximately 74 A. These results demonstrate that ouabain inhibits the (Na,K)-ATPase by causing a protein conformational change which extends an unusually large distance across the membrane.

Identification of proteins associated with apolipoprotein A-I-containing lipoproteins purified by selected-affinity immunosorption.

The isolation of apolipoprotein A-I-containing lipoproteins [Lp(A-I)] by selected-affinity immunosorption minimizes the loss of associated proteins that occurs during the isolation of high-density lipoproteins (HDL) by sequential ultracentrifugation. We have used two-dimensional gel electrophoretic analysis to separate the proteins associated with Lp(A-I). Using a combination of amino acid sequencing of transblotted proteins and Western blotting with specific antisera, we have identified a number of associated proteins. The positions of the apolipoproteins (apo) A-I, A-II, A-IV, C-III, D, and E were located on the gels. Lecithin-cholesterol acyltransferase and cholesteryl ester transfer protein were identified in association with Lp(A-I) to a greater extent than found associated with HDL after centrifugation. In addition to those proteins previously identified in association with HDL, we detected a number of plasma proteins associated with Lp(A-I), namely, fibrinogen, haptoglobin, proline-rich protein (C4b-binding protein), and apolipoprotein J (SP40,40 sulfated glycoprotein). The co-isolation of these proteins with Lp(A-I) does not appear to be an artifact in that they have very low affinity for a sham column containing covalently bound preimmune goat IgG in place of the anti-apoA-I IgG. These findings suggest that in addition to apolipoproteins that exist largely in association with lipoproteins there is another class of proteins which exist in lipoprotein-associated form and in the dispersed state. Detection and identification of these lipoprotein-associated proteins may aid in the mechanistic determination of a number of observed functions attributed to HDL.

Semi-preparative purification of recombinant human renin and prorenin.

Chinese hamster ovary (CHO) cells, transfected with a vector containing cDNA coding for preprorenin, have been shown to secrete authentic prorenin into the culture supernatant. Purification of the expressed prorenin and purification of active renin, generated by solid-phase trypsin treatment of the conditioned media, have been achieved by conventional chromatographic methods. Scale-up of the initial steps of these procedures is described, including the use of radial-flow columns and automation with fast protein liquid chromatography valves and pumps. This semi-preparative scheme has allowed hundreds of milligrams of both proteins to be isolated.

A molecular Einstein ring: imaging a starburst disk surrounding a quasi-stellar object.

Images of the molecular CO 2-1 line emission and the radio continuum emission from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein ring with a diameter of 1.5". These observations are modeled as a star-forming disk surrounding the QSO nucleus with a radius of 2 kiloparsecs. The implied massive star formation rate is 900 solar masses per year. At this rate, a substantial fraction of the stars in a large elliptical galaxy could form on a dynamical time scale of 108 years. The observation of active star formation in the host galaxy of a high-redshift QSO supports the hypothesis of coeval formation of supermassive black holes and stars in spheroidal galaxies.

Identification of an enzyme in human kidney that correctly processes prorenin.

Using pure recombinant human prorenin as a substrate, we have identified an enzyme in human kidney that accurately processes prorenin to active renin (EC 3.4.23.15). In the crude homogenate, the predominant activity of this potential renin-processing enzyme (RPE) converted the Mr 47,000 inactive prorenin to Mr 44,000 active renin and had a pH optimum of approximately 6. The activity was blocked by cysteine protease inhibitors, but not by pepstatin, EDTA, or serine protease inhibitors. This RPE activity was not detected in a similarly prepared homogenate of human chorion decidua tissue, which produces primarily prorenin, or in human plasma. The activity was purified 100-fold by ammonium sulfate precipitation, p-chloromercuribenzoate affinity chromatography, and chromatofocusing. The partially purified enzyme has a Mr of approximately 27,000 and an isoelectric point in the pH 4.8-5.6 range. The activity in the purified RPE preparation had the same pH optimum as that in crude homogenate, cleaved the prosegment at the same site used by the kidney in vivo based on amino-terminal sequencing of the processed renin, and did not degrade prorenin or renin. These data suggest that the cysteine protease we have isolated is a candidate for authentic renal RPE.