Period-luminosity relations for red supergiant variables - II. The distance to M101
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/313/4/868/3805165/313-4-868.pdf
Reference39 articles.
1. Ground-Based Discovery of Cepheids and Miras in M101
2. Discovery of Cepheids in M101
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1. The SN 2023ixf Progenitor in M101. I. Infrared Variability;The Astrophysical Journal;2023-10-30
2. SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova;The Astrophysical Journal Letters;2023-07-01
3. Properties of self-excited pulsations in 3D simulations of AGB stars and red supergiants;Astronomy & Astrophysics;2023-01
4. A Massive Star’s Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae;The Astrophysical Journal;2020-02-28
5. The period–luminosity relation of red supergiants with Gaia DR2;Monthly Notices of the Royal Astronomical Society;2019-06-10
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