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Cited by 347

The DOI matches its Crossref record; 40 of the 40 references it cites were found in a registry or an index.

PTF 11kx: A Type Ia Supernova with a Symbiotic Nova Progenitor

Open access
Dilday, B., Howell, D. A., Cenko, S. B., Silverman, J. M., Nugent, P. E., Sullivan, M., Ben-Ami, S., Bildsten, L., Bolte, M., Endl, M., Filippenko, A. V., Gnat, O., Horesh, A., Hsiao, E., Kasliwal, M. M., Kirkman, D., Maguire, K., Marcy, G. W., Moore, K., Pan, Y., Parrent, J. T., Podsiadlowski, P., Quimby, R. M., Sternberg, A., Suzuki, N., Tytler, D. R., Xu, D., Bloom, J. S., Gal-Yam, A., Hook, I. M., Kulkarni, S. R., Law, N. M., Ofek, E. O., Polishook, D., Poznanski, D.·2012·Science

Abstract

Stellar Explosions: Stars that are born with masses greater than eight times that of the Sun end their lives in luminous explosions known as supernovae. Over the past decade, access to improved sky surveys has revealed rare types of supernovae that are much more luminous than any of those that were known before. Gal-Yam (p. 927 ) reviews these superluminous events and groups them into three classes that share common observational and physical characteristics. Gamma-ray bursts are another type of extreme explosive events related to the death of massive stars, which occur once per day somewhere in the universe and produce short-lived bursts of gamma-ray light. Gehrels and Mészáros (p. 932 ) review what has been learned about these events since the launch of NASA's Swift (2004) and Fermi (2008) satellites. The current interpretation is that gamma-ray bursts are related to the formation of black holes. Type Ia supernovae are used as cosmological distance indicators. They are thought to be the result of the thermonuclear explosion of white dwarf stars in binary systems, but the nature of the stellar companion to the white dwarf is still debated. Dilday et al. (p. 942 ) report high-resolution spectroscopy of the supernova PTF 11kx, which was detected on 26 January 2011 by the Palomar Transient Factory survey. The data suggest a red giant star companion whose material got transferred to the white dwarf.

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Metadata

Authors
Dilday, B., Howell, D. A., Cenko, S. B., Silverman, J. M., Nugent, P. E., Sullivan, M., Ben-Ami, S., Bildsten, L., Bolte, M., Endl, M., Filippenko, A. V., Gnat, O., Horesh, A., Hsiao, E., Kasliwal, M. M., Kirkman, D., Maguire, K., Marcy, G. W., Moore, K., Pan, Y., Parrent, J. T., Podsiadlowski, P., Quimby, R. M., Sternberg, A., Suzuki, N., Tytler, D. R., Xu, D., Bloom, J. S., Gal-Yam, A., Hook, I. M., Kulkarni, S. R., Law, N. M., Ofek, E. O., Polishook, D., & Poznanski, D.
Venue
Science
Published
2012-08-24
Volume
337
Issue
6097
Pages
942-945
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2052024119
Cited by
347
References
40
FWCI
22.68
Type
journal article
Language
en
Open access
green

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The paper
Dilday, B., Howell, D. A., Cenko, S. B., Silverman, J. M., Nugent, P. E., Sullivan, M., Ben-Ami, S., Bildsten, L., Bolte, M., Endl, M., Filippenko, A. V., Gnat, O., Horesh, A., Hsiao, E., Kasliwal, M. M., Kirkman, D., Maguire, K., Marcy, G. W., Moore, K., . . . Poznanski, D. (2012). PTF 11kx: A Type Ia Supernova with a Symbiotic Nova Progenitor. Science. https://doi.org/10.1126/science.1219164

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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