Pismis 20 is a compact open cluster in Circinus . It is located at the heart of the Circinus OB1 association in the Norma arm of the Milky Way Galaxy. Pismis 20 is about 3,270 pc away and only about 5 million years old. HD 134959, a blue supergiant variable star also called CX Circinus, is the brightest star in Pismis 20.
Prominent stars
Star name
MV number
Effective temperature
Absolute magnitude
Bolometric magnitude
Mass (M ☉ )
Spectral type
Ref.
WR 67
11
56000
-4.03
-8
9
WN6-w
CX Circinus (HD 134959)
1
20900
-7.9
-9.8
50
B2.5Ia
6
42600
-4.2
-8.2
34
B
2
34400
-5.4
-8.8
34
O8.5I
3
28800
-5.5
-8.4
26
B0I
7
30200
-5
-8
23
B0III
4
29500
-5
-7.9
23
B0.2III
5
30200
-4.5
-7.5
20
B0III
References
^ "Pismis 20" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 30 December 2020.
Turner, David G. (1996). "PISMIS 20 - A Case Study of a Young Cluster" . Astronomical Journal . 111 : 828. Bibcode :1996AJ....111..828T . doi :10.1086/117829 .
Orsatti, A. M.; Vega, E. I.; Marraco, H. G. (2003). "Pismis 20: One or two clusters?" . Astronomy and Astrophysics . 408 : 135–140. Bibcode :2003A&A...408..135O . doi :10.1051/0004-6361:20030919 . hdl :11336/36974 – via 2003A&A...408..135O.
Sota, A.; Maíz Apellániz, J.; Morrell, N. I. ; Barbá, R. H.; Walborn, N. R.; Gamen, R. C.; Arias, J. I.; Alfaro, E. J.; Oskinova, L. M. (2019). "The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters". Astronomy & Astrophysics . A57 : 625. arXiv :1904.04687 . Bibcode :2019A&A...625A..57H . doi :10.1051/0004-6361/201834850 . S2CID 104292503 .
^ Massey, P.; Degioia-Eastwood, K. ; Waterhouse, E. (2001). "The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. II. Results from 12 Galactic Clusters and OB Associations". The Astronomical Journal . 121 (2): 1050–1070. arXiv :astro-ph/0010654 . Bibcode :2001AJ....121.1050M . doi :10.1086/318769 . S2CID 53345173 .
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