Draft:M10-VLA1
Appearance
![]() | This is a draft article. It is a work in progress open to editing by anyone. Please ensure core content policies are met before publishing it as a live Wikipedia article. Find sources: Google (books · news · scholar · free images · WP refs) · FENS · JSTOR · TWL Last edited by AluminiumWithAnI (talk | contribs) 2 days ago. (Update)
Finished drafting? or |
M10-VLA1 is a variable binary star in the globular cluster Messier 10 that is both a radio source and an X-ray source, situated in the equatorial constellation of Ophiuchus about 4,400 parsecs (14,000 light-years) distant. Discovered spectroscopically in 2018, the system was found to contain an unusual red straggler star orbiting an invisible companion of an uncertain nature.
Discovery
[edit]Properties
[edit]References
[edit]- Shishkovsky, Laura; Strader, Jay; Chomiuk, Laura; Bahramian, Arash; Tremou, Evangelia; Li, Kwan-Lok; Salinas, Ricardo; Tudor, Vlad; Miller-Jones, James C. A.; Maccarone, Thomas J.; Heinke, Craig O.; Sivakoff, Gregory R. (1 March 2018). "The MAVERIC Survey: A Red Straggler Binary with an Invisible Companion in the Galactic Globular Cluster M10". The Astrophysical Journal. 855 (1): 55. arXiv:1802.01704. doi:10.3847/1538-4357/aaadb1. ISSN 0004-637X.
- Rozyczka, M.; Pych, W.; Thompson, I.B.; Mazur, B. (2020). "The Clusters AgeS Experiment (CASE). Variable Stars in the Field of the Globular Cluster NGC 3201 - a Supplement". Acta Astronomica. 70 (4): 291–299. arXiv:2001.01529. doi:10.32023/0001-5237/70.4.3.
- "[SSC2020] M10-VLA1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 28 May 2025.