CWISEP J1047+5457
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ursa Major |
| Right ascension | 10h 47m 57.50s |
| Declination | +54° 57′ 42.17″ |
| Characteristics | |
| Evolutionary stage | brown dwarf |
| Spectral type | Y1[1] |
| Astrometry | |
| Proper motion (μ) | RA: -447.9 ±41.7 mas/yr[2] Dec.: -65.5 ±35.2 mas/yr[2] |
| Parallax (π) | 68.1 ± 4.9 mas[1] |
| Distance | 48 ± 3 ly (15 ± 1 pc) |
| Details | |
| Mass | 20.6 or 15.9[3] MJup |
| Radius | 0.94 ± 0.07 or 0.98 ± 0.07[3] RJup |
| Luminosity (bolometric) | 10-6.582 ± 0.063[1] L☉ |
| Temperature | 415+20 −22[1] K |
| Age | 6.73 or 5.01[3] Gyr |
| Other designations | |
CWISEP J104756.81+545741.6 | |
| Database references | |
| SIMBAD | data |
CWISEP J1047+5457 (CWISEP J104756.81+545741.6, CWISEP J1047+54) is a Y-dwarf discovered in 2020.[4]
CWISEP J1047+5457 was discovered in 2020 from a preliminary CatWISE catalog, initially determined to have a spectral type of Y0.[4] Follow-up observations with JWST spectroscopy (NIRSpec and MIRI) showed that it had a spectral type of Y1. The observations showed that it had unusually strong carbon monoxide and carbon dioxide absorption. This causes the Spitzer ch1-ch2 color to be extremely blue (2.47 ±0.19 mag) for its spectral type and explains the misidentification as a Y0 in the discovery paper. The strong absorption might be explained with extreme disequilibrium chemistry, low surface gravity, or a low carbon to oxygen ratio. Other molecules, such as water vapor, methane and ammonia are also detected in the spectra. Phosphine is not detected.[1]
See also
[edit]- List of Y-dwarfs
- CWISE J1055+5443 is another Y-dwarf with blue ch1-ch2 color, here this is explained with a young age
- List of star systems within 45–50 light-years
References
[edit]- ^ a b c d e Beiler, Samuel A.; Cushing, Michael C.; Kirkpatrick, J. Davy; Schneider, Adam C.; Mukherjee, Sagnick; Marley, Mark S.; Marocco, Federico; Smart, Richard L. (11 Jul 2024). "Precise Bolometric Luminosities and Effective Temperatures of 23 late-T and Y dwarfs Obtained with JWST". arXiv:2407.08518 [astro-ph.SR].
- ^ Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Bardalez Gagliuffi, Daniella C. (2021-03-01). "The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs". The Astrophysical Journal Supplement Series. 253 (1): 7. arXiv:2011.11616. Bibcode:2021ApJS..253....7K. doi:10.3847/1538-4365/abd107. ISSN 0067-0049.
- ^ a b c Zhijun, Tu; Shu, Wang; Liu, Jifeng (28 September 2024). "Physical Parameters and Properties of 20 Cold Brown Dwarfs in JWST". arXiv:2409.19191 [astro-ph].
- ^ a b Meisner, Aaron M.; Caselden, Dan; Kirkpatrick, J. Davy; Marocco, Federico; Gelino, Christopher R.; Cushing, Michael C.; Eisenhardt, Peter R. M.; Wright, Edward L.; Faherty, Jacqueline K.; Koontz, Renata; Marchese, Elijah J.; Khalil, Mohammed; Fowler, John W.; Schlafly, Edward F. (2020-02-01). "Expanding the Y Dwarf Census with Spitzer Follow-up of the Coldest CatWISE Solar Neighborhood Discoveries". The Astrophysical Journal. 889 (2): 74. arXiv:1911.12372. Bibcode:2020ApJ...889...74M. doi:10.3847/1538-4357/ab6215. ISSN 0004-637X.