Collinder 228 is an open cluster within the southern part of the Carina Nebula NGC 3372 , about 25' south of η Carinae .[ 2] It is probably composed of stars which recently formed from the material in the nebula. QZ Carinae is the brightest member of Collinder 228 with an apparent magnitude between 6.16–6.49 .[ 3]
Prominent stars in Collinder 228
Star name
FMF number
Effective temperature
Absolute magnitude
Bolometric magnitude
Mass (M ☉ )
Spectral type
Ref.
WR 24 (HD 93131)
3
50100
−7.34
−11.4
114
WN6ha-w
[ 4]
QZ Car (HD 93206)
33
30400 + 20000 + 34000 + 32900
−9.2 + 3 + 8.5 + 7
−10.6
27.1 + 6.5 + 25.4 + 17.1
O9.7I + B2V + O8III + O9V
[ 5] [ 6] [ 7]
HD 93632
92
45400
−6.1
−10.2
76
O5III(f)
[ 7]
V661 Car (HD 93130)
1
39900
−6.3
−10.1
68
O7II(f)
[ 7]
HD 305525
98
43600
−5.7
−9.8
58
O6V
[ 7]
97
46100
−4.8
−9
47
O5V
[ 7]
HD 93146
42400
−5.1
−9.1
44
O6.5V((f))
[ 7]
HD 305524
7
41000
−5.2
−9.1
42
O7V((f))
[ 7]
HD 93222
6
37200
−5.7
−9.3
42
O8III((f))
[ 7]
HD 305523
32
35700
−5.6
−9.1
38
O8.5III
[ 7]
HD 305532
38
43600
−4.4
−8.5
38
O6V((f))
[ 7]
HD 305438
24
38500
−4.6
−8.4
32
O8V
[ 7]
HD 93028
27
35700
−4.9
−8.4
30
O8.5III
[ 7]
HD 305518
22
34700
−5
−8.3
29
O9.5V
[ 7]
HD 93027
14
36000
−4.8
−8.3
29
O9V
[ 7]
39
37200
−4.6
−8.2
29
O8.5V((f))
[ 7]
HD 305539
94
37200
−4.4
−8.1
28
O8.5V
[ 7]
67
36000
−4.7
−8.2
28
O9V
[ 7]
HD 93576
93
36000
−4.7
−8.2
28
O9V
[ 7]
21
37200
−4.2
−7.8
27
O8.5V
[ 7]
HD 305536
5
34700
−4.7
−8.1
26
O9.5V
[ 7]
66
34700
−3.9
−7.3
22
O9.5V
[ 7]
12
20900
−6.1
−8
20
B2.5Ia:
[ 7]
See also
References
^ a b c d "Collinder 228" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 29 December 2020 .
^ Feinstein, A. (1995). "Open clusters in the Carina Nebula". Revista Mexicana de Astronomía y Astrofísica . Serie de Conferencias. 2 : 57. Bibcode :1995RMxAC...2...57F .
^ Samus, N.N.; Durlevich, O.V.; et al. (2009). General Catalogue of Variable Stars (Samus+ 2007–2013) (Report). VizieR On-line Data Catalog. Vol. 1. p. 02025. Bibcode :2009yCat....102025S . doi :10.1134/S1063772917010085 . B/GCVS. Originally published in Astronomy Reports (January 2017) DOI 10.1134/S1063772917010085
^ 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 .
^ Rainot, A.; Reggiani, M.; Sana, H.; Bodensteiner, J.; Gomez-Gonzalez, C.A.; Absil, O.; et al. (2020). "Carina High-contrast Imaging Project for Massive Stars (CHIPS). I. Methodology and proof of concept on QZ Car (≡ HD 93206)". Astronomy and Astrophysics . 640 : A15. arXiv :2006.01914 . Bibcode :2020A&A...640A..15R . doi :10.1051/0004-6361/201936448 . S2CID 219260368 .
^ Parkin, E.R.; Broos, P.S.; Townsley, L.K.; Pittard, J.M.; Moffat, A.F.J.; Nazé, Y.; et al. (2011). "X-ray emission from the double-binary OB-star system QZ Car (HD 93206)". The Astrophysical Journal Supplement . 194 (1). article 8. arXiv :1103.0794 . Bibcode :2011ApJS..194....8P . doi :10.1088/0067-0049/194/1/8 . S2CID 119292907 .
^ a b c d e f g h i j k l m n o p q r s t u v Massey, P.; de Gioia-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 .