SN 2013aa and SN 2017cbv:Two Sibling Type Ia Supernovae in the Spiral Galaxy NGC 5643

التفاصيل البيبلوغرافية
العنوان: SN 2013aa and SN 2017cbv:Two Sibling Type Ia Supernovae in the Spiral Galaxy NGC 5643
المؤلفون: Kevin Krisciunas, C. Gonzalez, Christopher R. Burns, Chris Ashall, Peter Hoeflich, Eric Hsiao, Nicholas B. Suntzeff, Joshua D. Simon, J. Vílchez, Maximilian Stritzinger, Jaime Vargas-González, S. Holmbo, Anthony L. Piro, David J. Sand, Syed Uddin, Mark M. Phillips, Charles D. Kilpatrick, Nahir Muñoz-Elgueta, Lluís Galbany, N. Ulloa, Ricardo Flores, Abdo Campillay, Peter J. Brown, Carlos Contreras, César Rojas-Bravo, Ryan J. Foley, Robert P. Kirshner, Nidia Morrell, Wendy L. Freedman
المصدر: Burns, C R, Ashall, C, Contreras, C, Brown, P, Stritzinger, M, Phillips, M M, Flores, R, Suntzeff, N B, Hsiao, E Y, Uddin, S, Simon, J D, Krisciunas, K, Campillay, A, Foley, R J, Freedman, W L, Galbany, L, González, C, Hoeflich, P, Holmbo, S, Kilpatrick, C D, Kirshner, R P, Morrell, N, Muñoz-Elgueta, N, Piro, A L, Rojas-Bravo, C, Sand, D, Vargas-González, J, Ulloa, N & Vilchez, J A 2020, ' SN 2013aa and SN 2017cbv : Two Sibling Type Ia Supernovae in the Spiral Galaxy NGC 5643 ', The Astrophysical Journal, vol. 895, no. 2, 118 . https://doi.org/10.3847/1538-4357/ab8e3e
The Astrophysical Journal
سنة النشر: 2020
مصطلحات موضوعية: 010504 meteorology & atmospheric sciences, Cepheid variable, Astrophysics::High Energy Astrophysical Phenomena, Galaxy distances, Photometric system, FOS: Physical sciences, Distance indicators, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 0103 physical sciences, Peculiar velocity, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Type Ia supernovae, Spiral galaxy, Cosmic distance ladder, Interstellar dust extinction, Astronomy and Astrophysics, Light curve, Astrophysics - Astrophysics of Galaxies, Galaxy, Supernova, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics - High Energy Astrophysical Phenomena
الوصف: We present photometric and spectroscopic observations of SN 2013aa and SN 2017cbv, two nearly identical type Ia supernovae (SNe Ia) in the host galaxy NGC 5643. The optical photometry has been obtained using the same telescope and instruments used by the Carnegie Supernova Project. This eliminates most instrumental systematics and provides light curves in a stable and well-understood photometric system. Having the same host galaxy also eliminates systematics due to distance and peculiar velocity, providing an opportunity to directly test the relative precision of SNe Ia as standard candles. The two SNe have nearly identical decline rates, negligible reddening, and remarkably similar spectra and, at a distance of $\sim 20$ Mpc, are ideal as potential calibrators for the absolute distance using primary indicators such as Cepheid variables. We discuss to what extent these two SNe can be considered twins and compare them with other supernova "siblings" in the literature and their likely progenitor scenarios. Using 12 galaxies that hosted 2 or more SNe~Ia, we find that when using SNe~Ia, and after accounting for all sources of observational error, one gets consistency in distance to 3 percent.
Accepted for publication in the Astrophysical Journal
وصف الملف: application/pdf
اللغة: English
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c6038e598d7510889ed9a6723492e4d
https://pure.au.dk/portal/da/publications/sn-2013aa-and-sn-2017cbv(184b3e52-8461-4e75-9f77-243a2b7b8181).html
حقوق: OPEN
رقم الأكسشن: edsair.doi.dedup.....5c6038e598d7510889ed9a6723492e4d
قاعدة البيانات: OpenAIRE