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1.
Philos Trans R Soc Lond B Biol Sci ; 367(1597): 1860-8, 2012 Jul 05.
Artículo en Inglés | MEDLINE | ID: mdl-22641824

RESUMEN

The structure and function of primate communication have attracted much attention, and vocal signals, in particular, have been studied in detail. As a general rule, larger social groups emit more types of vocal signals, including those conveying the presence of specific types of predators. The adaptive advantages of receiving and responding to alarm calls are expected to exert a selective pressure on the auditory system. Yet, the comparative biology of primate hearing is limited to select species, and little attention has been paid to the effects of social and vocal complexity on hearing. Here, we use the auditory brainstem response method to generate the largest number of standardized audiograms available for any primate radiation. We compared the auditory sensitivities of 11 strepsirrhine species with and without independent contrasts and show that social complexity explains a significant amount of variation in two audiometric parameters-overall sensitivity and high-frequency limit. We verified the generality of this latter result by augmenting our analysis with published data from nine species spanning the primate order. To account for these findings, we develop and test a model of social drive. We hypothesize that social complexity has favoured enhanced hearing sensitivities, especially at higher frequencies.


Asunto(s)
Percepción Auditiva/fisiología , Evolución Biológica , Potenciales Evocados Auditivos del Tronco Encefálico , Primates/fisiología , Adaptación Fisiológica , Animales , Audiometría de Respuesta Evocada/métodos , Audición/fisiología , Conducta Social , Medio Social , Especificidad de la Especie , Vocalización Animal/fisiología
2.
Biol Lett ; 8(4): 508-11, 2012 Aug 23.
Artículo en Inglés | MEDLINE | ID: mdl-22319094

RESUMEN

Few mammals-cetaceans, domestic cats and select bats and rodents-can send and receive vocal signals contained within the ultrasonic domain, or pure ultrasound (greater than 20 kHz). Here, we use the auditory brainstem response (ABR) method to demonstrate that a species of nocturnal primate, the Philippine tarsier (Tarsius syrichta), has a high-frequency limit of auditory sensitivity of ca 91 kHz. We also recorded a vocalization with a dominant frequency of 70 kHz. Such values are among the highest recorded for any terrestrial mammal, and a relatively extreme example of ultrasonic communication. For Philippine tarsiers, ultrasonic vocalizations might represent a private channel of communication that subverts detection by predators, prey and competitors, enhances energetic efficiency, or improves detection against low-frequency background noise.


Asunto(s)
Comunicación Animal , Potenciales Evocados Auditivos del Tronco Encefálico , Sonido , Tarsiidae/fisiología , Estimulación Acústica/métodos , Animales , Audición/fisiología , Localización de Sonidos , Especificidad de la Especie , Tarsiidae/psicología
3.
Pharmacogenomics ; 10(10): 1581-7, 2009 Oct.
Artículo en Inglés | MEDLINE | ID: mdl-19842931

RESUMEN

AIMS: A common, functionally significant polymorphism in GRK5 (Gln41Leu) encodes a gain-of-function enzyme that enhances desensitization of the beta(1)-adrenergic receptor. GRK5 Leu41 has been postulated to confer endogenous 'genetic beta-blockade' and contribute to an attenuated response to beta-blockers in black subjects. The effects of this GRK5 variant on sensitivity to a beta-blocker have not been studied in humans. We hypothesized that the GRK5 Gln41Leu variant contributes to interindividual variability in response to beta-blockade and to the ethnic difference in sensitivity between black and Caucasian individuals. MATERIALS & METHODS: We measured the heart rate at rest and during a graded incremental exercise in 154 healthy subjects (85 white and 69 black) before and after an oral administration of 25 mg atenolol. We determined the genotypes of GRK5 (Gln41Leu), beta(1)-adrenergic receptor (ADRB1 Ser49Gly and Arg389Gly) genotypes and plasma atenolol concentrations. The effects of genotype and covariates on sensitivity to atenolol, measured as the reduction in exercise-induced tachycardia, were determined using multiple regression analyses. RESULTS: The minor allele frequency of GRK5 Leu41 was 32.6% in blacks and 0% in whites. Black individuals were less sensitive to atenolol than white individuals (p < or = 0.011) but this was not explained by the GRK5 genotype. The GRK5 genotype had no effect on resting heart rate before (p = 0.61) and after adjustment for age, sex, ethnicity, atenolol concentrations, BMI and ADRB1 genotypes (p = 0.81). The decrease in heart rate after atenolol administration did not differ significantly according to the GRK5 genotype at rest or after exercise, before (all p > 0.14) and after statistical adjustment for covariates (all p > 0.17). CONCLUSION: The GRK5 Gln41Leu polymorphism does not affect sensitivity to the beta(1)-adrenergic blocker, atenolol, during acute physiological adrenergic stimulation, nor does it contribute to the ethnic differences in sensitivity to atenolol among black and Caucasian individuals.


Asunto(s)
Antagonistas de Receptores Adrenérgicos beta 1 , Antagonistas Adrenérgicos beta/farmacología , Quinasa 5 del Receptor Acoplado a Proteína-G/genética , Polimorfismo Genético/genética , Receptores Adrenérgicos beta 1/genética , Adulto , Alelos , Atenolol/farmacología , Población Negra , Electrocardiografía , Femenino , Frecuencia de los Genes , Variación Genética , Genotipo , Frecuencia Cardíaca/efectos de los fármacos , Humanos , Masculino , Farmacogenética/métodos , Taquicardia/etnología , Taquicardia/genética , Población Blanca
4.
Science ; 323(5915): 754-7, 2009 Feb 06.
Artículo en Inglés | MEDLINE | ID: mdl-19150809

RESUMEN

Massive stars produce so much light that the radiation pressure they exert on the gas and dust around them is stronger than their gravitational attraction, a condition that has long been expected to prevent them from growing by accretion. We present three-dimensional radiation-hydrodynamic simulations of the collapse of a massive prestellar core and find that radiation pressure does not halt accretion. Instead, gravitational and Rayleigh-Taylor instabilities channel gas onto the star system through nonaxisymmetric disks and filaments that self-shield against radiation while allowing radiation to escape through optically thin bubbles. Gravitational instabilities cause the disk to fragment and form a massive companion to the primary star. Radiation pressure does not limit stellar masses, but the instabilities that allow accretion to continue lead to small multiple systems.

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