Circumstellar Interaction of Type Ia Supernova SN 2002ic
SN 2002ic is a unique supernova which shows the typical spectral features of Type Ia supernovae (SNe Ia) near maximum light, but also apparent hydrogen features that have been absent in SNe Ia. We have calculated hydrodynamical models for the interaction between the SN Ia ejecta and the H-rich circu...
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| creator | Nomoto, Ken'ichi Suzuki, Tomoharu Deng, Jinsong Uenishi, Tatsuhiro Hachisu, Izumi Mazzali, Paolo |
| description | SN 2002ic is a unique supernova which shows the typical spectral features of
Type Ia supernovae (SNe Ia) near maximum light, but also apparent hydrogen
features that have been absent in SNe Ia. We have calculated hydrodynamical
models for the interaction between the SN Ia ejecta and the H-rich
circumstellar medium (CSM) to reproduce the observed features of SN 2002ic.
Based on our modeling, we suggest that CSM is aspherical (or highly clumpy) and
contains about 4-5 solar masses. Possible progenitor systems of SN 2002ic are
discussed. |
| doi_str_mv | 10.48550/arxiv.astro-ph/0406263 |
| format | Article |
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Type Ia supernovae (SNe Ia) near maximum light, but also apparent hydrogen
features that have been absent in SNe Ia. We have calculated hydrodynamical
models for the interaction between the SN Ia ejecta and the H-rich
circumstellar medium (CSM) to reproduce the observed features of SN 2002ic.
Based on our modeling, we suggest that CSM is aspherical (or highly clumpy) and
contains about 4-5 solar masses. Possible progenitor systems of SN 2002ic are
discussed.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0406263</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2004-06</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0406263$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0406263$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Nomoto, Ken'ichi</creatorcontrib><creatorcontrib>Suzuki, Tomoharu</creatorcontrib><creatorcontrib>Deng, Jinsong</creatorcontrib><creatorcontrib>Uenishi, Tatsuhiro</creatorcontrib><creatorcontrib>Hachisu, Izumi</creatorcontrib><creatorcontrib>Mazzali, Paolo</creatorcontrib><title>Circumstellar Interaction of Type Ia Supernova SN 2002ic</title><description>SN 2002ic is a unique supernova which shows the typical spectral features of
Type Ia supernovae (SNe Ia) near maximum light, but also apparent hydrogen
features that have been absent in SNe Ia. We have calculated hydrodynamical
models for the interaction between the SN Ia ejecta and the H-rich
circumstellar medium (CSM) to reproduce the observed features of SN 2002ic.
Based on our modeling, we suggest that CSM is aspherical (or highly clumpy) and
contains about 4-5 solar masses. Possible progenitor systems of SN 2002ic are
discussed.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzztrwzAUBWAtHUra31AtHZ3oeSONxfRhCM1Q7-ZaDyJwbCE7ofn3DWmmc5Zz4CPkhbO1MlqzDZbfdF7jvJSpyocNUwwEyEdi6lTc6TgvYRiw0GZcQkG3pGmkU6TtJQfaIP055VDG6Xxt31QwJpJ7Ig8Rhzk833NF2o_3tv6qdvvPpn7bVbi1sgLHrebXAZfcq6iNZw5E3GofrPUeILIYtLVKAhqpRQ-96h0PBjzvFUO5Iq__tzdAl0s6Yrl0N0iXD90dIv8A0JhE-Q</recordid><startdate>20040610</startdate><enddate>20040610</enddate><creator>Nomoto, Ken'ichi</creator><creator>Suzuki, Tomoharu</creator><creator>Deng, Jinsong</creator><creator>Uenishi, Tatsuhiro</creator><creator>Hachisu, Izumi</creator><creator>Mazzali, Paolo</creator><scope>GOX</scope></search><sort><creationdate>20040610</creationdate><title>Circumstellar Interaction of Type Ia Supernova SN 2002ic</title><author>Nomoto, Ken'ichi ; Suzuki, Tomoharu ; Deng, Jinsong ; Uenishi, Tatsuhiro ; Hachisu, Izumi ; Mazzali, Paolo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a793-6c1951002131d4f58d0c62f75de99dd66f0fe599436a8352b6b4bc1e86d1b40a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Nomoto, Ken'ichi</creatorcontrib><creatorcontrib>Suzuki, Tomoharu</creatorcontrib><creatorcontrib>Deng, Jinsong</creatorcontrib><creatorcontrib>Uenishi, Tatsuhiro</creatorcontrib><creatorcontrib>Hachisu, Izumi</creatorcontrib><creatorcontrib>Mazzali, Paolo</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Nomoto, Ken'ichi</au><au>Suzuki, Tomoharu</au><au>Deng, Jinsong</au><au>Uenishi, Tatsuhiro</au><au>Hachisu, Izumi</au><au>Mazzali, Paolo</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Circumstellar Interaction of Type Ia Supernova SN 2002ic</atitle><date>2004-06-10</date><risdate>2004</risdate><abstract>SN 2002ic is a unique supernova which shows the typical spectral features of
Type Ia supernovae (SNe Ia) near maximum light, but also apparent hydrogen
features that have been absent in SNe Ia. We have calculated hydrodynamical
models for the interaction between the SN Ia ejecta and the H-rich
circumstellar medium (CSM) to reproduce the observed features of SN 2002ic.
Based on our modeling, we suggest that CSM is aspherical (or highly clumpy) and
contains about 4-5 solar masses. Possible progenitor systems of SN 2002ic are
discussed.</abstract><doi>10.48550/arxiv.astro-ph/0406263</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.astro-ph/0406263 |
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| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | Circumstellar Interaction of Type Ia Supernova SN 2002ic |
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