Astronomy:WR 121-16
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Scutum |
| Right ascension | 18h 51m 39.7102s[1] |
| Declination | −05° 34′ 51.066″[1] |
| Apparent magnitude (V) | 14.02 (13.95 - 14.14)[2] |
| Characteristics | |
| Spectral type | WN7o/WC[2] |
| Apparent magnitude (J) | 11.369[3] |
| Apparent magnitude (K) | 10.609[3] |
| Astrometry | |
| Proper motion (μ) | RA: −2.450[1] mas/yr Dec.: −6.943[1] mas/yr |
| Parallax (π) | 0.0776 ± 0.0156[1] mas |
| Distance | 23,190[2] ly (7,110 pc) |
| Absolute magnitude (MV) | −3.955[2] |
| Details[2] | |
| Mass | 7.1+1.7 −1.1 M☉ |
| Radius | 4.14+1.4 −1.3 R☉ |
| Luminosity | 75,900+36,300 −22,200 L☉ |
| Temperature | 47,000+9,000 −5,000 K |
| Other designations | |
2MASS J18513970-0534510 | |
| Database references | |
| SIMBAD | data |
WR 121-16 is a transitional Wolf-Rayet star in the constellation of Scutum, near the Wild Duck Cluster (M11). It is located in the Far 3 kpc Arm of the Milky Way. It is very dim from Earth, having an apparent magnitude of about 14,[2] from being so reddened by interstellar extinction, and its distance of over 23,000 light years.[4] It is one of the dimmest known conventional Wolf-Rayet stars, with a luminosity of less than 76,000 times that of the Sun. WR 121-16 varies irregularly between magnitudes 13.95 and 14.14.[2]
WR 121-16 is a recent addition to the Wolf-Rayet Star Catalogue, being the 667th star added. It was discovered in August 2020.
Discovery
WR 121-16 was originally discovered as a ‘by-product’ of the LAMOST testing observations during the full moon nights, when the telescope was pointing to the open cluster M11, with WR 121-16 being about 42′ 24 apart from the centre of M11.[2]
Features
WR 121-16 is one of a few transitional Wolf-Rayet stars, which display both carbon and nitrogen emission, with a spectral type of WN7o/WC. Modelling the spectrum shows that WR 121-16 is not very luminous at all, with a luminosity of just 75,900 L☉, much less than most Wolf-Rayet stars. WR 121-16 has just over 7 solar masses, nearly all of which is helium. 1.5% of the star is composed of nitrogen, and 0.2% of it is composed of carbon.[2]
Strong stellar winds, typical of Wolf-Rayet stars, with a terminal velocity of 1,000 kilometers per second are causing WR 121-16 to lose 10−4.97 M☉/year,[2] much more than the Sun's (2-3) x 10−14 solar masses per year. The winds are so dense that the photosphere of the star is not visible. Its radius is defined for consistency with other Wolf-Rayet stars as being at an optical depth of 20, at about 4 R☉. A "transformed" radius at an optical depth of 2/3, more comparable to other types of star, is at about 6 R☉.[2]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 Zhang, Wei; Todt, Helge; Wu, Hong; Shi, Jianrong; Hsia, Chih-Hao; Wu, Yuzhong; Wu, Chaojian; Zhao, Yongheng et al. (2020-10-12). "A New Transition Wolf-Rayet WN/C Star in the Milky Way". The Astrophysical Journal 902 (1): 62. doi:10.3847/1538-4357/abb0e7. ISSN 1538-4357. Bibcode: 2020ApJ...902...62Z.
- ↑ 3.0 3.1 Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E. et al. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". CDS/ADC Collection of Electronic Catalogues 2246: II/246. Bibcode: 2003yCat.2246....0C. http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=II/246.
- ↑ "Wolf-Rayet Star Catalogue". http://pacrowther.staff.shef.ac.uk/WRcat/.
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