Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle

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MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFD

Edward F. Schlafly, Douglas P. Finkbeiner (2011)

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The Two Micron All Sky Survey (2MASS)

M. F. Skrutskie, R. Cutri, R. Stiening … (2006)

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Binary Interaction Dominates the Evolution of Massive Stars

H. Sana, S. E. de Mink, A. de Koter … (2012)

The presence of a nearby companion alters the evolution of massive stars in binary systems, leading to phenomena such as stellar mergers, x-ray binaries, and gamma-ray bursts. Unambiguous constraints on the fraction of massive stars affected by binary interaction were lacking. We simultaneously measured all relevant binary characteristics in a sample of Galactic massive O stars and quantified the frequency and nature of binary interactions. More than 70% of all massive stars will exchange mass with a companion, leading to a binary merger in one-third of the cases. These numbers greatly exceed previous estimates and imply that binary interaction dominates the evolution of massive stars, with implications for populations of massive stars and their supernovae.

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Author and article information

Contributors

M. Fraser: (View ORCID Profile)

T. Reynolds: (View ORCID Profile)

Journal

Title: Monthly Notices of the Royal Astronomical Society

Publisher: Oxford University Press (OUP)

ISSN (Print): 0035-8711

ISSN (Electronic): 1365-2966

Publication date Created: February 2018

Publication date Created: February 11 2018

Publication date Created: October 13 2017

Publication date Other: February 2018

Publication date (Print): February 11 2018

Publication date (Electronic): October 13 2017

Volume: 474

Issue: 1

Pages: 197-218

Affiliations

[1 ] INAF-Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy

[2 ] Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA

[3 ] Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University, 191 W. Woodruff Ave., Columbus, OH 43210, USA

[4 ] School of Physics, O’Brien Centre for Science North, University College Dublin, Belfield, Dublin 4, Ireland

[5 ] Institute of Astronomy, University of Cambridge, Madingley Road, CB3 0HA Cambridge, UK

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

[7 ] Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA

[8 ] Senior Miller Fellow, Miller Institute for Basic Research in Science, University of California, Berkeley, CA 94720, USA

[9 ] Astronomy Department, California Institute of Technology, Pasadena, CA 91125, USA

[10 ] Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland

[11 ] Nordic Optical Telescope, Apartado 474, E-38700 Santa Cruz de La Palma, Spain

[12 ] Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA

[13 ] Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, UK

[14 ] Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA

[15 ] Lunar and Planetary Lab, Department of Planetary Sciences, University of Arizona, Tucson, AZ 85721, USA

[16 ] Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[17 ] Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark

[18 ] Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100, Israel

[19 ] Gran Telescopio Canarias (GRANTECAN), Cuesta de San José s/n, E-38712 Breña Baja, La Palma, Spain

[20 ] Instituto de Astrofísica de Canarias, Vía Láctea s/n, E-38200 La Laguna, Tenerife, Spain

[21 ] Institut de Ciències de l’Espai (CSIC - IEEC), Campus UAB, Camì de Can Magrans S/N, E-08193 Cerdanyola (Barcelona), Spain

[22 ] Antelope Hills Observatory, 980 Antelope Drive West, Bennett, CO 80102, USA

[23 ] 66 Cours de Lassus, F-66000 Perpignan, France

[24 ] Department of Astronomy, The Oskar Klein Centre, AlbaNova University Center, Stockholm University, SE-10691 Stockholm, Sweden

[25 ] Applied Physics Department, Polytechnic Engineering School of Algeciras, University of Cádiz, Avenida Ramón Puyol S/N, E-11202 Algeciras, Spain

[26 ] Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA

[27 ] Groupe SNAude France, 364 Chemin de Notre Dame, F-06220 Vallauris, France

[28 ] Dipartimento di Fisica e Astronomia, Università di Padova, via Marzolo 8, I-35131 Padova, Italy

[29 ] Osservatorio Astronomico di Castelmartini, Via Bartolini 1317, I-51036 Larciano, Pistoia, Italy

[30 ] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

[31 ] Observation and Data Center for Cosmosciences, Faculty of Science, Hokkaido University, Kita-ku, Sapporo, Hokkaido 060-0810, Japan

[32 ] Nayoro Observatory, 157-1 Nisshin, Nayoro, Hokkaido 096-0066, Japan

[33 ] VSOLJ, Nishi juni-jou minami 3-1-5, Nayoro, Hokkaido 096-0022, Japan

Article

DOI: 10.1093/mnras/stx2668

SO-VID: 0c727027-b964-4ee7-8952-63e58fb1b740

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Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle

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Most cited references 120

MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFD

The Two Micron All Sky Survey (2MASS)

Binary Interaction Dominates the Evolution of Massive Stars

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