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Science
Resumen/Descripción – provisto por la editorial
No disponible.
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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
1880-
Cobertura temática
Tabla de contenidos
Melting around the margins
Sacha Vignieri; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 1552.5-1553
Reversing a regime shift (or not)
Sacha Vignieri; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 1552.6-1553
Probing an excitonic insulator
Sacha Vignieri; Jesse Smith (eds.)
Palabras clave: Multidisciplinary.
Pp. 1552.7-1553
An illuminating cosmic collision
Keith T. Smith
Palabras clave: Multidisciplinary.
Pp. 1554-1555
Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
D. A. Coulter
; R. J. Foley; C. D. Kilpatrick; M. R. Drout; A. L. Piro; B. J. Shappee; M. R. Siebert; J. D. Simon; N. Ulloa; D. Kasen; B. F. Madore; A. Murguia-Berthier; Y.-C. Pan; J. X. Prochaska; E. Ramirez-Ruiz; A. Rest; C. Rojas-Bravo
<jats:title>Photons from a gravitational wave event</jats:title> <jats:p> Two neutron stars merging together generate a gravitational wave signal and have also been predicted to emit electromagnetic radiation. When the gravitational wave event GW170817 was detected, astronomers rushed to search for the source using conventional telescopes (see the Introduction by Smith). Coulter <jats:italic>et al.</jats:italic> describe how the One-Meter Two-Hemispheres (1M2H) collaboration was the first to locate the electromagnetic source. Drout <jats:italic>et al.</jats:italic> present the 1M2H measurements of its optical and infrared brightness, and Shappee <jats:italic>et al.</jats:italic> report their spectroscopy of the event, which is unlike previously detected astronomical transient sources. Kilpatrick <jats:italic>et al.</jats:italic> show how these observations can be explained by an explosion known as a kilonova, which produces large quantities of heavy elements in nuclear reactions. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1556" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9811">1556</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1570" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0049">1570</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1574" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0186">1574</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1583" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0073">1583</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1556-1558
Illuminating gravitational waves: A concordant picture of photons from a neutron star merger
M. M. Kasliwal; E. Nakar; L. P. Singer; D. L. Kaplan; D. O. Cook; A. Van Sistine; R. M. Lau; C. Fremling; O. Gottlieb; J. E. Jencson; S. M. Adams; U. Feindt; K. Hotokezaka; S. Ghosh; D. A. Perley; P.-C. Yu; T. Piran; J. R. Allison; G. C. Anupama; A. Balasubramanian; K. W. Bannister; J. Bally; J. Barnes; S. Barway; E. Bellm; V. Bhalerao; D. Bhattacharya; N. Blagorodnova; J. S. Bloom; P. R. Brady; C. Cannella; D. Chatterjee; S. B. Cenko; B. E. Cobb; C. Copperwheat; A. Corsi; K. De; D. Dobie; S. W. K. Emery; P. A. Evans; O. D. Fox; D. A. Frail; C. Frohmaier; A. Goobar; G. Hallinan; F. Harrison; G. Helou; T. Hinderer; A. Y. Q. Ho; A. Horesh; W.-H. Ip; R. Itoh; D. Kasen; H. Kim; N. P. M. Kuin; T. Kupfer; C. Lynch; K. Madsen; P. A. Mazzali; A. A. Miller; K. Mooley; T. Murphy; C.-C. Ngeow; D. Nichols; S. Nissanke; P. Nugent; E. O. Ofek; H. Qi; R. M. Quimby; S. Rosswog; F. Rusu; E. M. Sadler; P. Schmidt; J. Sollerman; I. Steele; A. R. Williamson; Y. Xu; L. Yan; Y. Yatsu; C. Zhang; W. Zhao
<jats:title>GROWTH observations of GW170817</jats:title> <jats:p> The gravitational wave event GW170817 was caused by the merger of two neutron stars (see the Introduction by Smith). In three papers, teams associated with the GROWTH (Global Relay of Observatories Watching Transients Happen) project present their observations of the event at wavelengths from x-rays to radio waves. Evans <jats:italic>et al.</jats:italic> used space telescopes to detect GW170817 in the ultraviolet and place limits on its x-ray flux, showing that the merger generated a hot explosion known as a blue kilonova. Hallinan <jats:italic>et al.</jats:italic> describe radio emissions generated as the explosion slammed into the surrounding gas within the host galaxy. Kasliwal <jats:italic>et al.</jats:italic> present additional observations in the optical and infrared and formulate a model for the event involving a cocoon of material expanding at close to the speed of light, matching the data at all observed wavelengths. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1565" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9580">1565</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1579" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9855">1579</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1559" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9455">1559</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1559-1565
Swift and NuSTAR observations of GW170817: Detection of a blue kilonova
P. A. Evans; S. B. Cenko; J. A. Kennea; S. W. K. Emery; N. P. M. Kuin; O. Korobkin; R. T. Wollaeger; C. L. Fryer; K. K. Madsen; F. A. Harrison; Y. Xu; E. Nakar; K. Hotokezaka; A. Lien; S. Campana; S. R. Oates; E. Troja; A. A. Breeveld; F. E. Marshall; S. D. Barthelmy; A. P. Beardmore; D. N. Burrows; G. Cusumano; A. D’Aì; P. D’Avanzo; V. D’Elia; M. de Pasquale; W. P. Even; C. J. Fontes; K. Forster; J. Garcia; P. Giommi; B. Grefenstette; C. Gronwall; D. H. Hartmann; M. Heida; A. L. Hungerford; M. M. Kasliwal; H. A. Krimm; A. J. Levan; D. Malesani; A. Melandri; H. Miyasaka; J. A. Nousek; P. T. O’Brien; J. P. Osborne; C. Pagani; K. L. Page; D. M. Palmer; M. Perri; S. Pike; J. L. Racusin; S. Rosswog; M. H. Siegel; T. Sakamoto; B. Sbarufatti; G. Tagliaferri; N. R. Tanvir; A. Tohuvavohu
<jats:title>GROWTH observations of GW170817</jats:title> <jats:p> The gravitational wave event GW170817 was caused by the merger of two neutron stars (see the Introduction by Smith). In three papers, teams associated with the GROWTH (Global Relay of Observatories Watching Transients Happen) project present their observations of the event at wavelengths from x-rays to radio waves. Evans <jats:italic>et al.</jats:italic> used space telescopes to detect GW170817 in the ultraviolet and place limits on its x-ray flux, showing that the merger generated a hot explosion known as a blue kilonova. Hallinan <jats:italic>et al.</jats:italic> describe radio emissions generated as the explosion slammed into the surrounding gas within the host galaxy. Kasliwal <jats:italic>et al.</jats:italic> present additional observations in the optical and infrared and formulate a model for the event involving a cocoon of material expanding at close to the speed of light, matching the data at all observed wavelengths. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1565" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9580">1565</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1579" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9855">1579</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1559" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9455">1559</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1565-1570
Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
M. R. Drout; A. L. Piro; B. J. Shappee; C. D. Kilpatrick; J. D. Simon; C. Contreras; D. A. Coulter; R. J. Foley; M. R. Siebert; N. Morrell; K. Boutsia; F. Di Mille; T. W.-S. Holoien; D. Kasen; J. A. Kollmeier; B. F. Madore; A. J. Monson; A. Murguia-Berthier; Y.-C. Pan; J. X. Prochaska; E. Ramirez-Ruiz; A. Rest; C. Adams; K. Alatalo; E. Bañados; J. Baughman; T. C. Beers; R. A. Bernstein; T. Bitsakis; A. Campillay; T. T. Hansen; C. R. Higgs; A. P. Ji; G. Maravelias; J. L. Marshall; C. Moni Bidin; J. L. Prieto; K. C. Rasmussen; C. Rojas-Bravo; A. L. Strom; N. Ulloa; J. Vargas-González; Z. Wan; D. D. Whitten
<jats:title>Photons from a gravitational wave event</jats:title> <jats:p> Two neutron stars merging together generate a gravitational wave signal and have also been predicted to emit electromagnetic radiation. When the gravitational wave event GW170817 was detected, astronomers rushed to search for the source using conventional telescopes (see the Introduction by Smith). Coulter <jats:italic>et al.</jats:italic> describe how the One-Meter Two-Hemispheres (1M2H) collaboration was the first to locate the electromagnetic source. Drout <jats:italic>et al.</jats:italic> present the 1M2H measurements of its optical and infrared brightness, and Shappee <jats:italic>et al.</jats:italic> report their spectroscopy of the event, which is unlike previously detected astronomical transient sources. Kilpatrick <jats:italic>et al.</jats:italic> show how these observations can be explained by an explosion known as a kilonova, which produces large quantities of heavy elements in nuclear reactions. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1556" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9811">1556</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1570" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0049">1570</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1574" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0186">1574</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1583" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0073">1583</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1570-1574
Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger
B. J. Shappee; J. D. Simon; M. R. Drout; A. L. Piro; N. Morrell; J. L. Prieto; D. Kasen; T. W.-S. Holoien; J. A. Kollmeier; D. D. Kelson; D. A. Coulter; R. J. Foley; C. D. Kilpatrick; M. R. Siebert; B. F. Madore; A. Murguia-Berthier; Y.-C. Pan; J. X. Prochaska; E. Ramirez-Ruiz; A. Rest; C. Adams; K. Alatalo; E. Bañados; J. Baughman; R. A. Bernstein; T. Bitsakis; K. Boutsia; J. R. Bravo; F. Di Mille; C. R. Higgs; A. P. Ji; G. Maravelias; J. L. Marshall; V. M. Placco; G. Prieto; Z. Wan
<jats:title>Photons from a gravitational wave event</jats:title> <jats:p> Two neutron stars merging together generate a gravitational wave signal and have also been predicted to emit electromagnetic radiation. When the gravitational wave event GW170817 was detected, astronomers rushed to search for the source using conventional telescopes (see the Introduction by Smith). Coulter <jats:italic>et al.</jats:italic> describe how the One-Meter Two-Hemispheres (1M2H) collaboration was the first to locate the electromagnetic source. Drout <jats:italic>et al.</jats:italic> present the 1M2H measurements of its optical and infrared brightness, and Shappee <jats:italic>et al.</jats:italic> report their spectroscopy of the event, which is unlike previously detected astronomical transient sources. Kilpatrick <jats:italic>et al.</jats:italic> show how these observations can be explained by an explosion known as a kilonova, which produces large quantities of heavy elements in nuclear reactions. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1556" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9811">1556</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1570" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0049">1570</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1574" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0186">1574</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1583" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aaq0073">1583</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1574-1578
A radio counterpart to a neutron star merger
G. Hallinan; A. Corsi; K. P. Mooley; K. Hotokezaka; E. Nakar; M. M. Kasliwal; D. L. Kaplan; D. A. Frail; S. T. Myers; T. Murphy; K. De; D. Dobie; J. R. Allison; K. W. Bannister; V. Bhalerao; P. Chandra; T. E. Clarke; S. Giacintucci; A. Y. Q. Ho; A. Horesh; N. E. Kassim; S. R. Kulkarni; E. Lenc; F. J. Lockman; C. Lynch; D. Nichols; S. Nissanke; N. Palliyaguru; W. M. Peters; T. Piran; J. Rana; E. M. Sadler; L. P. Singer
<jats:title>GROWTH observations of GW170817</jats:title> <jats:p> The gravitational wave event GW170817 was caused by the merger of two neutron stars (see the Introduction by Smith). In three papers, teams associated with the GROWTH (Global Relay of Observatories Watching Transients Happen) project present their observations of the event at wavelengths from x-rays to radio waves. Evans <jats:italic>et al.</jats:italic> used space telescopes to detect GW170817 in the ultraviolet and place limits on its x-ray flux, showing that the merger generated a hot explosion known as a blue kilonova. Hallinan <jats:italic>et al.</jats:italic> describe radio emissions generated as the explosion slammed into the surrounding gas within the host galaxy. Kasliwal <jats:italic>et al.</jats:italic> present additional observations in the optical and infrared and formulate a model for the event involving a cocoon of material expanding at close to the speed of light, matching the data at all observed wavelengths. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1565" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9580">1565</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1579" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9855">1579</jats:related-article> , p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1559" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aap9455">1559</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6370" page="1554" related-article-type="in-this-issue" vol="358" xlink:href="10.1126/science.aar6069">1554</jats:related-article> </jats:p>
Palabras clave: Multidisciplinary.
Pp. 1579-1583