Alicante 8
| Alicante 8 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Scutum |
| Right ascension | 18h 34m 00s[1] |
| Declination | −07° 14′ 00″[1] |
| Distance | ~20 kly (~6–7 kpc[2]) |
| Apparent magnitude (V) | not visible[2] |
| Apparent dimensions (V) | <7′[2] |
| Physical characteristics | |
| Mass | 1–2 × 104 M☉ |
| Radius | <10 pc |
| Estimated age | 16–20 Mya[2] |
| Other designations | RSGC4 |
Alicante 8, also known as RSGC4, is a young massive open cluster belonging to the Milky Way galaxy. It was discovered in 2010 in the 2MASS survey data.[2] As of 2010, the only members of the cluster that are currently identified are 8–13 red supergiants—young massive stars undergoing helium burning in their cores. The cluster is located in the constellation Scutum at the distance of about 20–23 kly (6–7 kpc) from the Sun. It is likely situated at the intersection of the northern end of the Long Bar of the Milky Way and the inner portion of the Scutum–Centaurus Arm—one of the two major spiral arms.[2]
The age of Alicante 8 is estimated at 16–20 million years. The observed red supergiants with the mass of about 12 solar masses are type II supernova progenitors. The cluster is heavily obscured and have not been detected in the visible light. It lies close to other groupings of red supergiants known as RSGC1, Stephenson 2, and RSGC3. The mass of the open cluster is estimated at 10–20 thousand solar masses, which makes it one of the most massive open clusters in the Galaxy.[2]
References
- 1 2 "SIMBAD Astronomical Database". Results for RSGC 4. Retrieved 2010-11-14.
- 1 2 3 4 5 6 7 Negueruela, I.; González-Fernández, C.; Marco, A.; Clark, J. S.; Martínez-Núñez, S. (2010). "Another cluster of red supergiants close to RSGC1". Astronomy and Astrophysics. 513: A74. arXiv:1002.1823
. Bibcode:2010A&A...513A..74N. doi:10.1051/0004-6361/200913373.