Supernova progenitors, their variability and the Type IIP Supernova ASASSN-16fq in M66-Reference-Cited by-同舟云学术

Supernova progenitors, their variability and the Type IIP Supernova ASASSN-16fq in M66

Published:2017-02-24 Issue:3 Volume:467 Page:3347-3360
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kochanek C. S.¹²,Fraser M.³,Adams S. M.⁴,Sukhbold T.¹²,Prieto J. L.⁵⁶,Müller T.⁶⁷,Bock G.⁸,Brown J. S.¹,Dong Subo⁹,Holoien T. W.-S.¹,Khan R.¹⁰,Shappee B. J.¹¹,Stanek K. Z.¹²

Affiliation:

1. Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA

2. Center for Cosmology and AstroParticle Physics, The Ohio State University, 191 W. Woodruff Avenue, Columbus, OH 43210, USA

3. Institute of Astronomy, University of Cambridge, Madingley Rd, Cambridge CB3 0HA, UK

4. Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA

5. Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile

6. Millennium Institute of Astrophysics, Santiago 7591245, Chile

7. Instituto de Astrofísica, Pontifica Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile

8. Runaway Bay Observatory, 1 Lee Road, Runaway Bay, Queensland 4216, Australia

9. Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Road 5, Hai Dian District, Beijing 100871, China

10. Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195, USA

11. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA

Funder

NSF

NASA

DOE

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/467/3/3347/10875823/stx291.pdf

Reference106 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. LOSS's first supernova? New limits on the ‘impostor’ SN 1997bs

3. Almost gone: SN 2008S and NGC 300 2008OT-1 are fainter than their progenitors

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