The Early Light Curve of SN 2023bee: Constraining Type Ia Supernova Progenitors the Apian Way

被引：7

作者：

Hosseinzadeh, Griffin ^{[1
]}

Sand, David J. ^{[1
]}

Sarbadhicary, Sumit K. ^{[2
]}

Ryder, Stuart D. ^{[3
,4
]}

Jha, Saurabh W. ^{[5
]}

Dong, Yize ^{[6
]}

Bostroem, K. Azalee ^{[1
]}

Andrews, Jennifer E. ^{[7
]}

Hoang, Emily ^{[6
]}

Janzen, Daryl ^{[8
]}

Jencson, Jacob E. ^{[1
]}

Lundquist, Michael ^{[9
]}

Meza Retamal, Nicolas E. ^{[6
]}

Pearson, Jeniveve ^{[1
]}

Shrestha, Manisha ^{[1
]}

Valenti, Stefano ^{[6
]}

Wyatt, Samuel ^{[10
]}

Farah, Joseph ^{[11
,12
]}

Howell, D. Andrew ^{[11
,12
]}

McCully, Curtis ^{[11
,12
]}

Newsome, Megan ^{[11
,12
]}

Gonzalez, Estefania Padilla ^{[11
,12
]}

Pellegrino, Craig ^{[11
,12
]}

Terreran, Giacomo ^{[11
]}

Alzaabi, Muzoun ^{[1
]}

Green, Elizabeth M. ^{[1
]}

Gurney, Jessica L. ^{[1
]}

Milne, Peter A. ^{[1
]}

Ridenhour, Kaycee I. ^{[1
]}

Smith, Nathan ^{[1
]}

Robles, Paulina Soto ^{[1
]}

Kwok, Lindsey A. ^{[5
]}

Schwab, Michaela ^{[5
]}

Gromadzki, Mariusz ^{[13
]}

Buckley, David A. H. ^{[14
,15
,16
]}

Itagaki, Koichi ^{[17
]}

Hiramatsu, Daichi ^{[18
,19
]}

Chomiuk, Laura ^{[20
]}

Lundqvist, Peter ^{[21
]}

Haislip, Joshua ^{[22
]}

Kouprianov, Vladimir ^{[22
]}

Reichart, Daniel E. ^{[22
]}

机构：

[1] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA

[2] Ohio State Univ, Ctr Cosmol & Astro Particle Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA

[3] Macquarie Univ, Sch Math & Phys Sci, Sydney, NSW 2109, Australia

[4] Macquarie Univ, Astron Astrophys & Astrophoton Res Ctr, Sydney, NSW 2109, Australia

[5] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA

[6] Univ Calif Davis, Dept Phys & Astron, 1 Shields Ave, Davis, CA 95616 USA

[7] Gemini Observ, 670 North Aohoku Pl, Hilo, HI 96720 USA

[8] Univ Saskatchewan, Dept Phys & Engn Phys, 116 Sci Pl, Saskatoon, SK S7N 5E2, Canada

[9] WM Keck Observ, 65-1120 Mamalahoa Highway, Kamuela, HI 96743 USA

[10] Univ Washington, Dept Astron, 3910 15th Ave NE, Seattle, WA 98195 USA

[11] Las Cumbres Observ, 6740 Cortona Dr, Suite 102, Goleta, CA 93117 USA

[12] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[13] Univ Warsaw, Astron Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland

[14] South African Astron Observ, POB 9, ZA-7935 Observatory, South Africa

[15] Univ Free State, Dept Phys, POB 339, ZA-9300 Bloemfontein, South Africa

[16] Univ Cape Town, Dept Astron, Private Bag X3, ZA-7701 Rondebosch, South Africa

[17] Itagaki Astron Observ, Yamagata 9902492, Japan

[18] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[19] NSF Inst Artificial Intelligence & Fundamental Int, Cambridge, MA USA

[20] Michigan State Univ, Ctr Data Intens & Time Domain Astron, Dept Phys & Astron, E Lansing, MI 48824 USA

[21] Stockholm Univ, Albanova Univ Ctr, Oskar Klein Ctr, Dept Astron, SE-10691 Stockholm, Sweden

[22] Univ N Carolina, Dept Phys & Astron, 120 East Cameron Ave, Chapel Hill, NC 27599 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2023年 / 953卷 / 01期

基金：

新加坡国家研究基金会;

关键词：

PHOTOMETRIC STANDARD STARS; WHITE-DWARFS; NEBULAR SPECTROSCOPY; RADIO; SPECTRA; COMPANION; EMISSION; EXCESS; NEARBY; EJECTA;

D O I：

10.3847/2041-8213/ace7c0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present very early photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2023bee, starting about 8 hr after the explosion, which reveal a strong excess in the optical and nearest UV (U and UVW1) bands during the first several days of explosion. This data set allows us to probe the nature of the binary companion of the exploding white dwarf and the conditions leading to its ignition. We find a good match to the Kasen model in which a main-sequence companion star stings the ejecta with a shock as they buzz past. Models of double detonations, shells of radioactive nickel near the surface, interaction with circumstellar material, and pulsational delayed detonations do not provide good matches to our light curves. We also observe signatures of unburned material, in the form of carbon absorption, in our earliest spectra. Our radio nondetections place a limit on the mass-loss rate from the putative companion that rules out a red giant but allows a main-sequence star. We discuss our results in the context of other similar SNe Ia in the literature.

引用

页数：12

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