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Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No detectada desde mar. 1997 / hasta dic. 2023 Science Journals

Información

Tipo de recurso:

revistas

ISSN impreso

0036-8075

ISSN electrónico

1095-9203

Editor responsable

American Association for the Advancement of Science (AAAS)

País de edición

Estados Unidos

Fecha de publicación

Cobertura temática

naturales

Ciencias naturales

Tabla de contenidos

doi: 10.1126/science.346.6213.1074-h

Undercutting the surface keeps liquids at bay

Marc S. Lavine

Palabras clave: Multidisciplinary.

Pp. 1074.8-1074

doi: 10.1126/science.346.6213.1074-i

Cross talk between mitochondria and mitosis

Stella M. Hurtley

Palabras clave: Multidisciplinary.

Pp. 1074.9-1074

doi: 10.1126/science.2014.346.6213.twil

Editors' Choice

Marc S. Lavine; Guy Riddihough; L. Bryan Ray; Nicholas S. Wigginton; Sacha Vignieri; Peter Stern

Palabras clave: Multidisciplinary.

Pp. 1075-1075

doi: 10.1126/science.346.6213.1075-a

Up and down the raven social ladder

Guy Riddihough

Palabras clave: Multidisciplinary.

Pp. 1075.1-1075

doi: 10.1126/science.346.6213.1075-b

Turtles' breathing evolved at a turtle's pace

Sacha Vignieri

Palabras clave: Multidisciplinary.

Pp. 1075.2-1075

doi: 10.1126/science.346.6213.1075-c

Virtual reality changes neuronal firing

Peter Stern

Palabras clave: Multidisciplinary.

Pp. 1075.3-1075

doi: 10.1126/science.346.6213.1075-d

Looking at lipids with lasers

Nicholas S. Wigginton

Palabras clave: Multidisciplinary.

Pp. 1075.4-1075

doi: 10.1126/science.346.6213.1075-e

Insulin secretion organized in the nucleus

L. Bryan Ray

Palabras clave: Multidisciplinary.

Pp. 1075.5-1075

doi: 10.1126/science.346.6213.1075-f

Sorting cells by subpopulations

Marc S. Lavine

Palabras clave: Multidisciplinary.

Pp. 1075.6-1075

doi: 10.1126/science.1256183

Black hole lightning due to particle acceleration at subhorizon scales

J. Aleksić; S. Ansoldi; L. A. Antonelli; P. Antoranz; A. Babic; P. Bangale; J. A. Barrio; J. Becerra González; W. Bednarek; E. Bernardini; B. Biasuzzi; A. Biland; O. Blanch; S. Bonnefoy; G. Bonnoli; F. Borracci; T. Bretz; E. Carmona; A. Carosi; P. Colin; E. Colombo; J. L. Contreras; J. Cortina; S. Covino; P. Da Vela; F. Dazzi; A. De Angelis; G. De Caneva; B. De Lotto; E. de Oña Wilhelmi; C. Delgado Mendez; D. Dominis Prester; D. Dorner; M. Doro; S. Einecke; D. Eisenacher; D. Elsaesser; M. V. Fonseca; L. Font; K. Frantzen; C. Fruck; D. Galindo; R. J. García López; M. Garczarczyk; D. Garrido Terrats; M. Gaug; N. Godinović; A. González Muñoz; S. R. Gozzini; D. Hadasch; Y. Hanabata; M. Hayashida; J. Herrera; D. Hildebrand; J. Hose; D. Hrupec; W. Idec; V. Kadenius; H. Kellermann; K. Kodani; Y. Konno; J. Krause; H. Kubo; J. Kushida; A. La Barbera; D. Lelas; N. Lewandowska; E. Lindfors; S. Lombardi; F. Longo; M. López; R. López-Coto; A. López-Oramas; E. Lorenz; I. Lozano; M. Makariev; K. Mallot; G. Maneva; N. Mankuzhiyil; K. Mannheim; L. Maraschi; B. Marcote; M. Mariotti; M. Martínez; D. Mazin; U. Menzel; J. M. Miranda; R. Mirzoyan; A. Moralejo; P. Munar-Adrover; D. Nakajima; A. Niedzwiecki; K. Nilsson; K. Nishijima; K. Noda; R. Orito; A. Overkemping; S. Paiano; M. Palatiello; D. Paneque; R. Paoletti; J. M. Paredes; X. Paredes-Fortuny; M. Persic; J. Poutanen; P. G. Prada Moroni; E. Prandini; I. Puljak; R. Reinthal; W. Rhode; M. Ribó; J. Rico; J. Rodriguez Garcia; S. Rügamer; T. Saito; K. Saito; K. Satalecka; V. Scalzotto; V. Scapin; C. Schultz; T. Schweizer; S. N. Shore; A. Sillanpää; J. Sitarek; I. Snidaric; D. Sobczynska; F. Spanier; V. Stamatescu; A. Stamerra; T. Steinbring; J. Storz; M. Strzys; L. Takalo; H. Takami; F. Tavecchio; P. Temnikov; T. Terzić; D. Tescaro; M. Teshima; J. Thaele; O. Tibolla; D. F. Torres; T. Toyama; A. Treves; M. Uellenbeck; P. Vogler; R. Zanin; M. Kadler; R. Schulz; E. Ros; U. Bach; F. Krauß; J. Wilms

<jats:p>Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescopes, revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20% of the gravitational radius of its central black hole. We suggest that the emission is associated with pulsar-like particle acceleration by the electric field across a magnetospheric gap at the base of the radio jet.</jats:p>

Palabras clave: Multidisciplinary.

Pp. 1080-1084