Westerlund 1-237

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Stern
Westerlund 1-237
Westerlund 1.jpg
Image of the super star cluster Westerlund 1 . Wd 1-237 is the bright reddish star below the center of the picture
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation altar
Right ascension 16 h 47 m 3.11 s
declination -45 ° 52 ′ 19 ″
Apparent brightness 19.01 mag
Typing
Spectral class M3Ia
Astrometry
Physical Properties
radius 1245  R
Luminosity

2.3 * 10 5  L

Effective temperature 3,600  K
Other names
and catalog entries
2MASS catalog 2MASS J16470309-4552189 [1]

Westerlund 1-237 or W237 is an extreme red supergiant belonging to the spectral class M3Ia. With an estimated diameter of 1245 solar radii, a luminosity of 234,000 L and an effective temperature of 3,600 K, it is one of the largest known stars . It is located in the star cluster Westerlund 1 in the constellation Altar , where it is one of a total of 4 known red giants ( Westerlund 1-26 , Westerlund 1-20, Westerlund 1-237, Westerlund 1-75). Westerlund 1-237 is surrounded by an elliptical radio nebula, which is similar in mass to that of W20 and W26, and is comparable to that of VY Canis Majoris.

Individual evidence

  1. ^ Cl * Westerlund 1 W 237. In: Simbad. Retrieved June 28, 2020 (English).
  2. Thomas KT Fok, Jun-ichi Nakashima, Bosco HK Yung, Chih-Hao Hsia, Shuji Deguchi: Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters . In: ApJ . tape 760 , no. 1 , November 2012, ISSN  0004-637X , p. 65 , doi : 10.1088 / 0004-637X / 760/1/65 ( harvard.edu [accessed June 28, 2020]).
  3. APOD: 2017 June 20 - The Massive Stars in Westerlund 1. Retrieved June 28, 2020 .
  4. SM Dougherty, JS Clark, I. Negueruela, T. Johnson, JM Chapman: Radio emission from the massive stars in the Galactic Super Star Cluster Westerlund 1 . In: Astronomy and Astrophysics . tape 511 , February 2010, ISSN  0004-6361 , p. A58 , doi : 10.1051 / 0004-6361 / 200913505 , arxiv : 0912.4165 .