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

Autor: 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
Jazyk: angličtina
Rok vydání: 2020
Předmět:
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
Zdroj: 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
DOI: 10.3847/1538-4357/ab8e3e
Popis: 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
Databáze: OpenAIRE