ORCID Profile
0000-0001-8135-6612
Current Organisation
University of Colorado at Boulder
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Publisher: American Astronomical Society
Date: 12-08-2020
Publisher: American Astronomical Society
Date: 15-03-2017
Publisher: American Astronomical Society
Date: 18-11-2019
Publisher: American Astronomical Society
Date: 19-04-2017
Publisher: American Astronomical Society
Date: 26-07-2019
Publisher: American Astronomical Society
Date: 02-04-2015
Publisher: American Astronomical Society
Date: 09-10-2014
Publisher: American Astronomical Society
Date: 21-10-2014
Publisher: American Astronomical Society
Date: 05-02-2018
Publisher: American Astronomical Society
Date: 28-11-2016
Publisher: American Astronomical Society
Date: 10-2022
Publisher: American Association for the Advancement of Science (AAAS)
Date: 22-12-2017
Abstract: 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 et al. 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 et al. describe radio emissions generated as the explosion slammed into the surrounding gas within the host galaxy. Kasliwal et al. 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. Science , this issue p. 1565 , p. 1579 , p. 1559 see also p. 1554
Publisher: American Astronomical Society
Date: 09-11-2020
Publisher: American Astronomical Society
Date: 14-10-2019
Location: United States of America
Location: United States of America
No related grants have been discovered for JOHN BALLY.