Platais 8, also known as the a Carinae cluster or HIP 45080 Cluster is a small and faint open cluster located in the southern constellation Carina. It is estimated to be 440 light years distant based on parallax measurements.[1]
The cluster was first noticed by astronomer Imants Platais in 1998.[4] A 2005 paper suggests that Platais 8 might have formed near the area where the Scorpius-Centaurus association is located. [5] The SIMBAD database lists the cluster having 28,185 members[6] but the majority of the stars are field stars. In fact, there are only 32 members physically associated with the cluster.[1] The cluster has a combined mass of 546 M☉ and a radius of 37.2 light years. Platais 8 is rather young, with an age of only 60 million years.[3]
Members
These are the members of the cluster as identified by Canat-Gaudin et al. (2018)
Name | mv | MK Type | Dist. (ly) | Notes |
---|---|---|---|---|
HD 76230 | 6.57 | A0 V | 410 | Binary |
HD 78802 | 7.33 | A2 IV | 467 | |
HD 76413 | 7.48 | A3 V | 417 | |
HD 80628 | 7.57 | A0/1 V | 442 | |
HD 78761 | 7.68 | A2 V | 454 | |
HD 78027 | 7.88 | A1 V | 444 |
The cluster also has one potential stream star located in Volans[1] and was considered to be a background object prior to 2020.
Name | mv | MK Type | Dist. (ly) | Notes |
---|---|---|---|---|
HD 71863 | 5.94 | G8/K0 III | 421 | HR 3346 |
References
- ^ a b c d e f g Cantat-Gaudin, T.; Anders, F. (January 2020). "Clusters and mirages: cataloguing stellar aggregates in the Milky Way". Astronomy & Astrophysics. 633: A99. arXiv:1911.07075. Bibcode:2020A&A...633A..99C. doi:10.1051/0004-6361/201936691. ISSN 0004-6361.
- ^ a b Piskunov, A. E.; Schilbach, E.; Kharchenko, N. V.; Röser, S.; Scholz, R.-D. (26 March 2007). "Towards absolute scales for the radii and masses of open clusters". Astronomy & Astrophysics. 468 (1): 151–161. arXiv:astro-ph/0702517. Bibcode:2007A&A...468..151P. doi:10.1051/0004-6361:20077073. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Vande Putte, D.; Garnier, T. P.; Ferreras, I.; Mignani, R. P.; Cropper, Mark (6 September 2010). "A kinematic study of open clusters: implications for their origin". Monthly Notices of the Royal Astronomical Society. 407 (4): 2109–2121. arXiv:0912.0695. Bibcode:2010MNRAS.407.2109V. doi:10.1111/j.1365-2966.2010.17025.x. ISSN 0035-8711.
- ^ Platais, Imants; Kozhurina-Platais, Vera; van Leeuwen, Floor (November 1998). "A Search for Star Clusters from the ]Hipparcos Data". The Astronomical Journal. 116 (5): 2423–2430. Bibcode:1998AJ....116.2423P. doi:10.1086/300606. ISSN 0004-6256.
- ^ Piskunov, A. E.; Kharchenko, N. V.; Röser, S.; Schilbach, E.; Scholz, R.-D. (16 December 2005). "Revisiting the population of Galactic open clusters". Astronomy & Astrophysics. 445 (2): 545–565. arXiv:astro-ph/0508575. Bibcode:2006A&A...445..545P. doi:10.1051/0004-6361:20053764. eISSN 1432-0746. ISSN 0004-6361.
- ^ "Cl Platais 8". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 7 January 2021.
- ^ Cantat-Gaudin, T.; Jordi, C.; Vallenari, A.; Bragaglia, A.; Balaguer-Núñez, L.; Soubiran, C.; Bossini, D.; Moitinho, A.; Castro-Ginard, A.; Krone-Martins, A.; Casamiquela, L.; Sordo, R.; Carrera, R. (October 2018). "A Gaia DR2 view of the open cluster population in the Milky Way". Astronomy & Astrophysics. 618: A93. arXiv:1805.08726. Bibcode:2018A&A...618A..93C. doi:10.1051/0004-6361/201833476. ISSN 0004-6361.
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