The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?
Abstract
Wide-field optical surveys have begun to uncover large samples of fast (trise ≲ 5 d), luminous (Mpeak < -18), blue transients. While commonly attributed to the breakout of a supernova shock into a dense wind, the great distances to the transients of this class found so far have hampered detailed investigation of their properties. We present photometry and spectroscopy from a comprehensive worldwide campaign to observe AT 2018cow (ATLAS 18qqn), the first fast-luminous optical transient to be found in real time at low redshift. Our first spectra (<2 days after discovery) are entirely featureless. A very broad absorption feature suggestive of near-relativistic velocities develops between 3 and 8 days, then disappears. Broad emission features of H and He develop after >10 days. The spectrum remains extremely hot throughout its evolution, and the photospheric radius contracts with time (receding below R < 1014 cm after 1 month). Furthermore, this behavior does not match that of any known supernova, although a relativistic jet within a fallback supernova could explain some of the observed features. Alternatively, the transient could originate from the disruption of a star by an intermediate-mass black hole, although this would require long-lasting emission of highly super-Eddington thermal radiation. Inmore »
- Authors:
-
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- Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK
- Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK, Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str 1, D-84741 Garching, Germany
- Division of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA
- Astrophysics Science Division, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA, Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA
- Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, DK-2100 Copenhagen, Denmark, Department of Astronomy, University of Maryland, College Park, MD 20742, USA
- Indian Institute of Astrophysics, II Block Koramangala, Bengaluru 560034, India, Joint Astronomy Programme, Department of Physics, Indian Institute of Science, Bengaluru 560012, India
- Kavli IPMU (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan, Department of Physics, Faculty of Science and Engineering, Konan University, 8-9-1 Okamoto, Kobe, Hyogo 658-8501, Japan
- Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, 04510 México, CDMX, México
- Indian Institute of Astrophysics, II Block Koramangala, Bengaluru 560034, India
- Department of Physics, Florida State Universiy, Tallahassee, FL 32306, USA
- Physics Department, Indian Institute of Technology Bombay, Powai, Mumbai 400076, India
- Department of Astronomy, University of California, Berkeley, CA 94720, USA
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
- The Oskar Klein Centre, Department of Physics, AlbaNova, Stockholm University, SE-106 91 Stockholm, Sweden
- Department of Astronomy/Mount Laguna Observatory, San Diego State University, 5500 Campanile Drive, San Diego, CA 92812-1221, USA
- Department of Physics, School of Science, Tokyo Institute of Technology, 2-12-1 Ohokayama, Meguro, Tokyo 152-8551, Japan
- Division of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA, Caltech Optical Observatories, California Institute of Technology, Pasadena, CA 91125, USA
- Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan
- Division of Physics, Math, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA, Center for Data Driven Discovery, California Institute of Technology, Pasadena, CA 91125, USA
- Graduate Institute of Astronomy, National Central University, 32001 Taipei , Taiwan
- Soka University of America, 1 University Drive, Aliso Viejo, CA 92656, USA
- INAF OAS, Via Piero Gobetti, 101, I-40129 Bologna, Italy
- Kavli IPMU (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan, Department of Astronomy/Mount Laguna Observatory, San Diego State University, 5500 Campanile Drive, San Diego, CA 92812-1221, USA
- Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, DK-2100 Copenhagen, Denmark, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
- Instituto de Astronomía UNAM, Unidad Académica en Ensenada, 22860 Ensenada BC, México
- The Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, SE-106 91 Stockholm, Sweden
- Yale-NUS College, 16 College Avenue West, Singapore 138527, Singapore
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1491926
- Alternate Identifier(s):
- OSTI ID: 1571983
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 484 Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Oxford University Press
- Country of Publication:
- United Kingdom
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Black hole; stars; supernovae: general; supernova: individual: AT2018cow
Citation Formats
Perley, Daniel A., Mazzali, Paolo A., Yan, Lin, Cenko, S. Bradley, Gezari, Suvi, Taggart, Kirsty, Blagorodnova, Nadia, Fremling, Christoffer, Mockler, Brenna, Singh, Avinash, Tominaga, Nozomu, Tanaka, Masaomi, Watson, Alan M., Ahumada, Tomás, Anupama, G. C., Ashall, Chris, Becerra, Rosa L., Bersier, David, Bhalerao, Varun, Bloom, Joshua S., Butler, Nathaniel R., Copperwheat, Chris, Coughlin, Michael W., De, Kishalay, Drake, Andrew J., Duev, Dmitry A., Frederick, Sara, González, J. Jesús, Goobar, Ariel, Heida, Marianne, Ho, Anna Y. Q., Horst, John, Hung, Tiara, Itoh, Ryosuke, Jencson, Jacob E., Kasliwal, Mansi M., Kawai, Nobuyuki, Khanam, Tanazza, Kulkarni, Shrinivas R., Kumar, Brajesh, Kumar, Harsh, Kutyrev, Alexander S., Lee, William H., Maeda, Keiichi, Mahabal, Ashish, Murata, Katsuhiro L., Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Pian, Elena, Quimby, Robert, Ramirez-Ruiz, Enrico, Richer, Michael G., Román-Zúñiga, Carlos G., Sahu, D. K., Srivastav, Shubham, Socia, Quentin, Sollerman, Jesper, Tachibana, Yutaro, Taddia, Francesco, Tinyanont, Samaporn, Troja, Eleonora, Ward, Charlotte, Wee, Jerrick, and Yu, Po-Chieh. The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?. United Kingdom: N. p., 2018.
Web. doi:10.1093/mnras/sty3420.
Perley, Daniel A., Mazzali, Paolo A., Yan, Lin, Cenko, S. Bradley, Gezari, Suvi, Taggart, Kirsty, Blagorodnova, Nadia, Fremling, Christoffer, Mockler, Brenna, Singh, Avinash, Tominaga, Nozomu, Tanaka, Masaomi, Watson, Alan M., Ahumada, Tomás, Anupama, G. C., Ashall, Chris, Becerra, Rosa L., Bersier, David, Bhalerao, Varun, Bloom, Joshua S., Butler, Nathaniel R., Copperwheat, Chris, Coughlin, Michael W., De, Kishalay, Drake, Andrew J., Duev, Dmitry A., Frederick, Sara, González, J. Jesús, Goobar, Ariel, Heida, Marianne, Ho, Anna Y. Q., Horst, John, Hung, Tiara, Itoh, Ryosuke, Jencson, Jacob E., Kasliwal, Mansi M., Kawai, Nobuyuki, Khanam, Tanazza, Kulkarni, Shrinivas R., Kumar, Brajesh, Kumar, Harsh, Kutyrev, Alexander S., Lee, William H., Maeda, Keiichi, Mahabal, Ashish, Murata, Katsuhiro L., Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Pian, Elena, Quimby, Robert, Ramirez-Ruiz, Enrico, Richer, Michael G., Román-Zúñiga, Carlos G., Sahu, D. K., Srivastav, Shubham, Socia, Quentin, Sollerman, Jesper, Tachibana, Yutaro, Taddia, Francesco, Tinyanont, Samaporn, Troja, Eleonora, Ward, Charlotte, Wee, Jerrick, & Yu, Po-Chieh. The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?. United Kingdom. https://doi.org/10.1093/mnras/sty3420
Perley, Daniel A., Mazzali, Paolo A., Yan, Lin, Cenko, S. Bradley, Gezari, Suvi, Taggart, Kirsty, Blagorodnova, Nadia, Fremling, Christoffer, Mockler, Brenna, Singh, Avinash, Tominaga, Nozomu, Tanaka, Masaomi, Watson, Alan M., Ahumada, Tomás, Anupama, G. C., Ashall, Chris, Becerra, Rosa L., Bersier, David, Bhalerao, Varun, Bloom, Joshua S., Butler, Nathaniel R., Copperwheat, Chris, Coughlin, Michael W., De, Kishalay, Drake, Andrew J., Duev, Dmitry A., Frederick, Sara, González, J. Jesús, Goobar, Ariel, Heida, Marianne, Ho, Anna Y. Q., Horst, John, Hung, Tiara, Itoh, Ryosuke, Jencson, Jacob E., Kasliwal, Mansi M., Kawai, Nobuyuki, Khanam, Tanazza, Kulkarni, Shrinivas R., Kumar, Brajesh, Kumar, Harsh, Kutyrev, Alexander S., Lee, William H., Maeda, Keiichi, Mahabal, Ashish, Murata, Katsuhiro L., Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Pian, Elena, Quimby, Robert, Ramirez-Ruiz, Enrico, Richer, Michael G., Román-Zúñiga, Carlos G., Sahu, D. K., Srivastav, Shubham, Socia, Quentin, Sollerman, Jesper, Tachibana, Yutaro, Taddia, Francesco, Tinyanont, Samaporn, Troja, Eleonora, Ward, Charlotte, Wee, Jerrick, and Yu, Po-Chieh. Sat .
"The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?". United Kingdom. https://doi.org/10.1093/mnras/sty3420.
@article{osti_1491926,
title = {The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?},
author = {Perley, Daniel A. and Mazzali, Paolo A. and Yan, Lin and Cenko, S. Bradley and Gezari, Suvi and Taggart, Kirsty and Blagorodnova, Nadia and Fremling, Christoffer and Mockler, Brenna and Singh, Avinash and Tominaga, Nozomu and Tanaka, Masaomi and Watson, Alan M. and Ahumada, Tomás and Anupama, G. C. and Ashall, Chris and Becerra, Rosa L. and Bersier, David and Bhalerao, Varun and Bloom, Joshua S. and Butler, Nathaniel R. and Copperwheat, Chris and Coughlin, Michael W. and De, Kishalay and Drake, Andrew J. and Duev, Dmitry A. and Frederick, Sara and González, J. Jesús and Goobar, Ariel and Heida, Marianne and Ho, Anna Y. Q. and Horst, John and Hung, Tiara and Itoh, Ryosuke and Jencson, Jacob E. and Kasliwal, Mansi M. and Kawai, Nobuyuki and Khanam, Tanazza and Kulkarni, Shrinivas R. and Kumar, Brajesh and Kumar, Harsh and Kutyrev, Alexander S. and Lee, William H. and Maeda, Keiichi and Mahabal, Ashish and Murata, Katsuhiro L. and Neill, James D. and Ngeow, Chow-Choong and Penprase, Bryan and Pian, Elena and Quimby, Robert and Ramirez-Ruiz, Enrico and Richer, Michael G. and Román-Zúñiga, Carlos G. and Sahu, D. K. and Srivastav, Shubham and Socia, Quentin and Sollerman, Jesper and Tachibana, Yutaro and Taddia, Francesco and Tinyanont, Samaporn and Troja, Eleonora and Ward, Charlotte and Wee, Jerrick and Yu, Po-Chieh},
abstractNote = {Wide-field optical surveys have begun to uncover large samples of fast (trise ≲ 5 d), luminous (Mpeak < -18), blue transients. While commonly attributed to the breakout of a supernova shock into a dense wind, the great distances to the transients of this class found so far have hampered detailed investigation of their properties. We present photometry and spectroscopy from a comprehensive worldwide campaign to observe AT 2018cow (ATLAS 18qqn), the first fast-luminous optical transient to be found in real time at low redshift. Our first spectra (<2 days after discovery) are entirely featureless. A very broad absorption feature suggestive of near-relativistic velocities develops between 3 and 8 days, then disappears. Broad emission features of H and He develop after >10 days. The spectrum remains extremely hot throughout its evolution, and the photospheric radius contracts with time (receding below R < 1014 cm after 1 month). Furthermore, this behavior does not match that of any known supernova, although a relativistic jet within a fallback supernova could explain some of the observed features. Alternatively, the transient could originate from the disruption of a star by an intermediate-mass black hole, although this would require long-lasting emission of highly super-Eddington thermal radiation. In either case, AT 2018cow suggests that the population of fast luminous transients represents a new class of astrophysical event. Intensive follow-up of this event in its late phases, and of any future events found at comparable distance, will be essential to better constrain their origins.},
doi = {10.1093/mnras/sty3420},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 484,
place = {United Kingdom},
year = {Sat Dec 22 00:00:00 EST 2018},
month = {Sat Dec 22 00:00:00 EST 2018}
}
https://doi.org/10.1093/mnras/sty3420
Web of Science
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