A repeating fast radio burst associated with a persistent radio source.

The dispersive sweep of fast radio bursts (FRBs) has been used to probe the ionized baryon content of the intergalactic medium1, which is assumed to dominate the total extragalactic dispersion. Although the host-galaxy contributions to the dispersion measure appear to be small for most FRBs2, in at least one case there is evidence for an extreme magneto-ionic local environment3,4 and a compact persistent radio source5. Here we report the detection and localization of the repeating FRB 20190520B, which is co-located with a compact, persistent radio source and associated with a dwarf host galaxy of high specific-star-formation rate at a redshift of 0.241 ± 0.001. The estimated host-galaxy dispersion measure of approximately [Formula: see text] parsecs per cubic centimetre, which is nearly an order of magnitude higher than the average of FRB host galaxies2,6, far exceeds the dispersion-measure contribution of the intergalactic medium. Caution is thus warranted in inferring redshifts for FRBs without accurate host-galaxy identifications.

An early transition to magnetic supercriticality in star formation.

Magnetic fields have an important role in the evolution of interstellar medium and star formation1,2. As the only direct probe of interstellar field strength, credible Zeeman measurements remain sparse owing to the lack of suitable Zeeman probes, particularly for cold, molecular gas3. Here we report the detection of a magnetic field of +3.8 ± 0.3 microgauss through the H I narrow self-absorption (HINSA)4,5 towards L15446,7-a well-studied prototypical prestellar core in an early transition between starless and protostellar phases8-10 characterized by a high central number density11 and a low central temperature12. A combined analysis of the Zeeman measurements of quasar H I absorption, H I emission, OH emission and HINSA reveals a coherent magnetic field from the atomic cold neutral medium (CNM) to the molecular envelope. The molecular envelope traced by the HINSA is found to be magnetically supercritical, with a field strength comparable to that of the surrounding diffuse, magnetically subcritical CNM despite a large increase in density. The reduction of the magnetic flux relative to the mass, which is necessary for star formation, thus seems to have already happened during the transition from the diffuse CNM to the molecular gas traced by the HINSA. This is earlier than envisioned in the classical picture where magnetically supercritical cores capable of collapsing into stars form out of magnetically subcritical envelopes13,14.

A bimodal burst energy distribution of a repeating fast radio burst source.

The event rate, energy distribution and time-domain behaviour of repeating fast radio bursts (FRBs) contain essential information regarding their physical nature and central engine, which are as yet unknown1,2. As the first precisely localized source, FRB 121102 (refs. 3-5) has been extensively observed and shows non-Poisson clustering of bursts over time and a power-law energy distribution6-8. However, the extent of the energy distribution towards the fainter end was not known. Here we report the detection of 1,652 independent bursts with a peak burst rate of 122 h-1, in 59.5 hours spanning 47 days. A peak in the isotropic equivalent energy distribution is found to be approximately 4.8 × 1037 erg at 1.25 GHz, below which the detection of bursts is suppressed. The burst energy distribution is bimodal, and well characterized by a combination of a log-normal function and a generalized Cauchy function. The large number of bursts in hour-long spans allows sensitive periodicity searches between 1 ms and 1,000 s. The non-detection of any periodicity or quasi-periodicity poses challenges for models involving a single rotating compact object. The high burst rate also implies that FRBs must be generated with a high radiative efficiency, disfavouring emission mechanisms with large energy requirements or contrived triggering conditions.

lncRNA-RMRP promotes proliferation, migration and invasion of bladder cancer via miR-206.

OBJECTIVE: The incidence of bladder cancer (BC) is common in the world, but its detail mechanisms for occurrence and development remain unclear. Recently, long non-coding RNAs (lncRNAs) have been observed to play an important role in many different diseases. In this research, we mainly explored the role of the RNA component of mitochondrial RNA processing endoribonuclease (lncRNA-RMRP) in bladder cancer. MATERIALS AND METHODS: We used qRT-PCR to detect the expression of lncRNA-RMRP in bladder cancer patients and tumor cells, and the clinical significance was also analyzed. The methyl thiazolyl tetrazolium (MTT) assay was used to detect the cell proliferation, and we used transwell to detect the migration and invasion, after the lncRNA RMRP was inhibited. Western-blot was used to measure the relative protein expression level in bladder cancer cells after transfection with siRNA-NC or siRNA-RMRP. RESULTS: We found that the lncRNA RMRP was highly expressed in bladder cancer tissue, compared with adjacent tissue. We also found that the expression of RMRP was closely related with the size, lymph node metastasis and survival time of patients. What's more, RMRP could promote the proliferation, migration and invasion of BC cell lines via regulating miR-206 as a sponge. CONCLUSIONS: According to the results, we found that lncRNA RMRP was closely related to the progression of bladder cancer, which could be a potential target for treating BC patients.

First Report of Bacterial Blight of Guar Caused by Xanthomonas axonopodis pv. cyamopsidis in China.

Bacterial blight was observed on field-grown guar (Cyamopsis tetragonoloba L.) for the first time in China. The disease outbreak occurred in the Xinjiang Uyghur Autonomous Region after several weeks of unusually heavy rains during late summer 2013. The disease incidence was generally 40 to 50%, although values as high as 80% were observed in several fields. Initial field symptoms included water-soaked spots on leaves, pods, petioles, and stems. During later stages of infection, the color of the spots became dark. We also observed large, angular, necrotic lesions at leaf tips, black streaks on petioles and stems, split stems, defoliation, wilting or top withering, vascular necrosis, and dieback. Samples of diseased leaves, stems, petioles, pods, and seeds were surface sterilized, ground, and then plated onto King's B medium. Plates were incubated at 28°C for 72 h. Fifteen bacterial strains with yellow-pigmented, opaque, and round colonies were isolated. These strains were aerobic, gram-negative rods with a single, polar flagellum. They were positive for H2S, esculin, oxidase, tobacco hypersensitivity, indole production from tryptophan, nitrate reduction to nitrite, and the utilization of glucose, mannose, trehalose, galactose, and starch. The maximum salt tolerance of the strains was 2 to 3%. Pathogenicity tests using eight strains were conducted in July 2013. A bacterial culture was suspended in sterile water with a final concentration of 108 CFU/ml. Eight 4-week-old guar plants were inoculated by (i) spraying the bacterial suspension on the leaves until runoff, or (ii) puncturing the stems with a needle that had been dipped into the bacterial suspension. Sterile water was used as a negative control. Plants were kept in a mist room with 100% relative humidity for 24 h. Stem and leaf symptoms similar to those of the original plants were observed on the inoculated guar plants within 10 days of inoculation. No symptoms developed on the negative control plants. Yellow bacterial colonies re-isolated from inoculated plant tissues were morphologically identical to the original. 16S rDNA was amplified using universal primers (Pa 5'-AGTTTGATCCTGGCTCAG-3' and Ph 5'-TACCTTGTTACGACTTCGTCCCA-3') and sequenced. A BLAST search of the NCBI GenBank database indicated that the 16S rDNA sequences of three strains (accession nos. KF563926, KF563927, and KF563928) had 99.9% identity to Xanthomonas axonopodis strain XV938 (AF123091). Under greenhouse conditions, bacterial strains wilted asparagus bean and pea but rarely infected bean, kidney bean, faba bean, mung bean, soybean, red bean, pea, garbanzo bean, and peanut. Based on morphology, pathogenicity tests, 16S rDNA sequencing, and host plant specificity, the pathogen was confirmed as X. axonopodis pv. cyamopsidis (synonym: X. campestris pv. cyamopsidis [Patel et al., 1953]). To our knowledge, this is the first report of bacterial blight of guar caused by X. axonopodis pv. cyamopsidis in China. Guar has recently been introduced in Xinjiang Province. Our findings indicate that bacterial blight may pose a threat to the economic sustainability of guar production in the region. References: (1) I. A. Milyutina et a1. FEMS Microbiol. Lett. 239:17, 2004. (2) I. M. G. Almeida et al. Summa Phytopathol. 18:255, 1992. (3) J. D. Mihail et al. Plant Dis. 69:811, 1985.