Astronomy:NGC 3293
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| NGC 3293 | |
|---|---|
 NGC 3293 taken by the Wide Field Imager on the MPG/ESO 2.2-meter telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Carina[1] |
| Right ascension | 10h 35m 24s[2] |
| Declination | −58° 14′[2] |
| Distance | 8,400 ly (2,590 pc)[3] |
| Apparent magnitude (V) | 4.7[1] |
| Apparent dimensions (V) | 8.2′[4] |
| Physical characteristics | |
| Mass | 1457[3] M☉ |
| Radius | 13.2 ly[4] |
| Estimated age | 12 ± 3 Myr[3] |
| Other designations | Cr 224 |
NGC 3293 is an open cluster of stars in the Constellation of Carina.[1] It was discovered by Nicolas-Louis de Lacaille in 1751.[5] This cluster consists of more than 100 stars brighter than 14th magnitude in a 10 arc minute field, the brightest of which are blue supergiants of apparent magnitude 6.5 and 6.7. There is also a 7th magnitude pulsating red supergiant, V361 Carinae.[6]
NGC 3293 is associated with the open cluster NGC 3324. Both are fairly young, at around 12 million years old. They show some degree of mass segregation, with more massive stars concentrated near their centers. Neither are dynamically relaxed.[3]
References
- ↑ 1.0 1.1 1.2 Finlay, Warren H. (2014). Concise Catalogue of Deep-Sky Objects. The Patrick Moore Practical Astronomy Series (2nd ed.). Springer Cham. p. 244. doi:10.1007/978-3-319-03170-5. ISBN 978-3-319-03169-9.
- ↑ 2.0 2.1 Kharchenko, N. V.; Piskunov, A. E.; Schilbach, E.; Röser, S.; Scholz, R.-D. (2013). "Global survey of star clusters in the Milky Way. II. The catalogue of basic parameters". Astronomy & Astrophysics 558: A53. doi:10.1051/0004-6361/201322302. Bibcode: 2013A&A...558A..53K.
- ↑ 3.0 3.1 3.2 3.3 Bisht, D.; Zhu, Qingfeng; Yadav, R K S.; Ganesh, Shashikiran; Rangwal, Geeta; Durgapal, Alok; Sariya, Devesh P.; Jiang, Ing-Guey (2021). "Multicolour photometry and Gaia EDR3 astrometry of two couples of binary clusters (NGC 5617 and Trumpler 22) and (NGC 3293 and NGC 3324)". Monthly Notices of the Royal Astronomical Society 503 (4): 5929–5947. doi:10.1093/mnras/stab691.
- ↑ 4.0 4.1 Baume, G.; Vázquez, R. A.; Carraro, G.; Feinstein, A. (2003). "Photometric study of the young open cluster NGC 3293". Astronomy and Astrophysics 402 (2): 531–540. doi:10.1051/0004-6361:20030223. Bibcode: 2003A&A...402..549B.
- ↑ Seligman, Courtney. "NGC Objects: NGC 3250 - 3299". http://cseligman.com/text/atlas/ngc32a.htm#3293.
- ↑ Dufton, P. L.; Smartt, S. J.; Lee, J. K.; Ryans, R. S. I.; Hunter, I.; Evans, C. J.; Herrero, A.; Trundle, C. et al. (2006). "The VLT-FLAMES survey of massive stars: Stellar parameters and rotational velocities in NGC 3293, NGC 4755 and NGC 6611". Astronomy and Astrophysics 457 (1): 265–280. doi:10.1051/0004-6361:20065392. Bibcode: 2006A&A...457..265D.
External links
- NGC 3293 @ SEDS NGC objects pages
- NASA Astronomy Picture of the Day: NGC 3293: A Bright Young Open Cluster (29 March 1998)
- NASA Astronomy Picture of the Day: NGC 3293: A Bright Young Star Cluster (6 April 2015)
Template:NGC objects:3000-3499
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