 Ross 19A (bright star) and Ross 19B (marked with a blue cross-hair) Credit: NASA WISE & unWISE (Meisner et al. 2022) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Triangulum |
| Ross 19A | |
| Right ascension | 02h 19m 03.0092s |
| Declination | +35° 21′ 18.601″ |
| Apparent magnitude (V) | 12.70 [1] |
| Ross 19B | |
| Right ascension | 02h 19m 48.68s |
| Declination | +35° 18′ 45.3″ |
| Characteristics | |
| Evolutionary stage | red dwarf + brown dwarf |
| Spectral type | M3.5 [1] + T9-Y0 [2] |
| Astrometry | |
| Ross 19A | |
| Radial velocity (Rv) | -27.80 ± 0.14 km/s |
| Proper motion (μ) |
RA: 670.532 ± 0.042
mas/
yr
[3] Dec.: -427.412 ± 0.040 mas/ yr [3] |
| Parallax (π) | 57.3276 ± 0.0398 mas [3] |
| Distance | 56.89 ± 0.04
ly (17.44 ± 0.01 pc) |
| Ross 19B | |
| Proper motion (μ) |
RA: 673.2 ± 46.4
mas/
yr
[3] Dec.: -504.4 ± 57.0 mas/ yr [3] |
| Distance | 17.58 ± 3.75 [3] pc |
| Details [3] | |
| Ross 19A | |
| Mass | 0.362 ± 0.007 M☉ |
| Radius | 3.38 ± 0.03 RJup |
| Temperature | 3481 ± 49 K |
| Metallicity [Fe/H] | -0.40 ± 0.12 dex |
| Age | 7.2+3.8 −3.6 Gyr |
| Ross 19B | |
| Mass | 15-40 MJup |
| Temperature | 500+115 −100 K |
| Position (relative to Ross 19A) [3] | |
| Component | Ross 19B |
| Angular distance | 568 ″ |
| Projected separation | 9900 AU |
| Other designations | |
| Ross 19B: CWISE J021948.68+351845.3 | |
| Database references | |
| Ross 19A | |
| SIMBAD | data |
| Ross 19B | |
| SIMBAD | data |
Ross 19 is a red dwarf of spectral type M3.5. [1] In 2021 it was discovered that Ross 19 has a companion, which is a cold brown dwarf. Ross 19B is likely the coldest brown dwarf found around a main-sequence star, as of July 2024. [3]
Ross 19A was discovered in 1925 by Frank E. Ross as a proper-motion star with the help of the Yerkes Observatory and archived plates by E. E. Barnard. [4] In 1985 the first spectral information was published by W. P. Bidelman, based on observations by G. P. Kuiper, which reported the star to have a V magnitude of 12.70 and a spectral type of M3.5. [1] In 2020 the star was observed at the Lick Observatory and with IRTF. Ross 19A has a mass of about 0.36 M☉ and has an age between 3.6 and 11 billion years. It has a sub-solar metallicity and has a temperature of about 3500 Kelvin. In TESS and ZTF light curves it does not show any variability and does not show any flares. [3]
Ross 19B (also called CWISE J021948.68+351845.3) was initially found in the Backyard Worlds project by the citizen scientists Samuel Goodman, Léopold Gramaize, Austin Rothermich, and Hunter Brooks. It was then observed by the professional astronomers of the paper lead by Adam C. Schneider with the Keck Observatory in 2020, measuring a J-band magnitude of 21.14 ± 0.02. The researchers calculated that Ross 19B has a 100% probability to be bound to Ross 19A. Ross 19B has a very low temperature of about 400–615 kelvins (127–342 °C; 260–647 °F), making it either a late T-dwarf or a Y-dwarf. It has a mass between 15 and 40 MJ, making it a brown dwarf. Its wide separation results in an extremely low gravitational binding energy. It is suggested that Ross 19B has a sub-solar metallicity similar to the red dwarf. [3] Later observation with Gemini North showed a Y-band magnitude of 21.86 ± 0.06. This showed that the spectral type is likely between T9 and Y0. [2] A JWST program is dedicated to observe Ross 19B in Cycle 3. [5]
- List of Y-dwarfs
- Wolf 1130C - another cold metal-poor companion
- WD 0806-661B - a Y-dwarf companion to a white dwarf
- ^ a b c d Bidelman, W. P. (1985-10-01). "G.P. Kuiper's spectral classifications of proper-motion stars". The Astrophysical Journal Supplement Series. 59: 197–227. Bibcode: 1985ApJS...59..197B. doi: 10.1086/191069. ISSN 0067-0049.
- ^ a b Meisner, Aaron M.; Leggett, S. K.; Logsdon, Sarah E.; Schneider, Adam C.; Tremblin, Pascal; Phillips, Mark (2023-08-01). "Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs". The Astronomical Journal. 166 (2): 57. arXiv: 2301.09817. Bibcode: 2023AJ....166...57M. doi: 10.3847/1538-3881/acdb68. ISSN 0004-6256.
- ^ a b c d e f g h i Schneider, Adam C.; Meisner, Aaron M.; Gagné, Jonathan; Faherty, Jacqueline K.; Marocco, Federico; Burgasser, Adam J.; Kirkpatrick, J. Davy; Kuchner, Marc J.; Gramaize, Léopold; Rothermich, Austin; Brooks, Hunter; Vrba, Frederick J.; Bardalez Gagliuffi, Daniella; Caselden, Dan; Cushing, Michael C. (2021-11-01). "Ross 19B: An Extremely Cold Companion Discovered via the Backyard Worlds: Planet 9 Citizen Science Project". The Astrophysical Journal. 921 (2): 140. arXiv: 2108.05321. Bibcode: 2021ApJ...921..140S. doi: 10.3847/1538-4357/ac1c75. ISSN 0004-637X.
- ^ Ross, Frank E. (1925-11-01). "New proper-motion stars, (first list)". The Astronomical Journal. 36: 96–99. Bibcode: 1925AJ.....36...96R. doi: 10.1086/104687. ISSN 0004-6256.
- ^ "5118 Program Information". www.stsci.edu. Retrieved 2024-07-21.
Ross 19A (bright star) and Ross 19B (marked with a blue cross-hair) Credit: NASA WISE & unWISE (Meisner et al. 2022) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Triangulum |
| Ross 19A | |
| Right ascension | 02h 19m 03.0092s |
| Declination | +35° 21′ 18.601″ |
| Apparent magnitude (V) | 12.70 [1] |
| Ross 19B | |
| Right ascension | 02h 19m 48.68s |
| Declination | +35° 18′ 45.3″ |
| Characteristics | |
| Evolutionary stage | red dwarf + brown dwarf |
| Spectral type | M3.5 [1] + T9-Y0 [2] |
| Astrometry | |
| Ross 19A | |
| Radial velocity (Rv) | -27.80 ± 0.14 km/s |
| Proper motion (μ) |
RA: 670.532 ± 0.042
mas/
yr
[3] Dec.: -427.412 ± 0.040 mas/ yr [3] |
| Parallax (π) | 57.3276 ± 0.0398 mas [3] |
| Distance | 56.89 ± 0.04
ly (17.44 ± 0.01 pc) |
| Ross 19B | |
| Proper motion (μ) |
RA: 673.2 ± 46.4
mas/
yr
[3] Dec.: -504.4 ± 57.0 mas/ yr [3] |
| Distance | 17.58 ± 3.75 [3] pc |
| Details [3] | |
| Ross 19A | |
| Mass | 0.362 ± 0.007 M☉ |
| Radius | 3.38 ± 0.03 RJup |
| Temperature | 3481 ± 49 K |
| Metallicity [Fe/H] | -0.40 ± 0.12 dex |
| Age | 7.2+3.8 −3.6 Gyr |
| Ross 19B | |
| Mass | 15-40 MJup |
| Temperature | 500+115 −100 K |
| Position (relative to Ross 19A) [3] | |
| Component | Ross 19B |
| Angular distance | 568 ″ |
| Projected separation | 9900 AU |
| Other designations | |
| Ross 19B: CWISE J021948.68+351845.3 | |
| Database references | |
| Ross 19A | |
| SIMBAD | data |
| Ross 19B | |
| SIMBAD | data |
Ross 19 is a red dwarf of spectral type M3.5. [1] In 2021 it was discovered that Ross 19 has a companion, which is a cold brown dwarf. Ross 19B is likely the coldest brown dwarf found around a main-sequence star, as of July 2024. [3]
Ross 19A was discovered in 1925 by Frank E. Ross as a proper-motion star with the help of the Yerkes Observatory and archived plates by E. E. Barnard. [4] In 1985 the first spectral information was published by W. P. Bidelman, based on observations by G. P. Kuiper, which reported the star to have a V magnitude of 12.70 and a spectral type of M3.5. [1] In 2020 the star was observed at the Lick Observatory and with IRTF. Ross 19A has a mass of about 0.36 M☉ and has an age between 3.6 and 11 billion years. It has a sub-solar metallicity and has a temperature of about 3500 Kelvin. In TESS and ZTF light curves it does not show any variability and does not show any flares. [3]
Ross 19B (also called CWISE J021948.68+351845.3) was initially found in the Backyard Worlds project by the citizen scientists Samuel Goodman, Léopold Gramaize, Austin Rothermich, and Hunter Brooks. It was then observed by the professional astronomers of the paper lead by Adam C. Schneider with the Keck Observatory in 2020, measuring a J-band magnitude of 21.14 ± 0.02. The researchers calculated that Ross 19B has a 100% probability to be bound to Ross 19A. Ross 19B has a very low temperature of about 400–615 kelvins (127–342 °C; 260–647 °F), making it either a late T-dwarf or a Y-dwarf. It has a mass between 15 and 40 MJ, making it a brown dwarf. Its wide separation results in an extremely low gravitational binding energy. It is suggested that Ross 19B has a sub-solar metallicity similar to the red dwarf. [3] Later observation with Gemini North showed a Y-band magnitude of 21.86 ± 0.06. This showed that the spectral type is likely between T9 and Y0. [2] A JWST program is dedicated to observe Ross 19B in Cycle 3. [5]
- List of Y-dwarfs
- Wolf 1130C - another cold metal-poor companion
- WD 0806-661B - a Y-dwarf companion to a white dwarf
- ^ a b c d Bidelman, W. P. (1985-10-01). "G.P. Kuiper's spectral classifications of proper-motion stars". The Astrophysical Journal Supplement Series. 59: 197–227. Bibcode: 1985ApJS...59..197B. doi: 10.1086/191069. ISSN 0067-0049.
- ^ a b Meisner, Aaron M.; Leggett, S. K.; Logsdon, Sarah E.; Schneider, Adam C.; Tremblin, Pascal; Phillips, Mark (2023-08-01). "Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs". The Astronomical Journal. 166 (2): 57. arXiv: 2301.09817. Bibcode: 2023AJ....166...57M. doi: 10.3847/1538-3881/acdb68. ISSN 0004-6256.
- ^ a b c d e f g h i Schneider, Adam C.; Meisner, Aaron M.; Gagné, Jonathan; Faherty, Jacqueline K.; Marocco, Federico; Burgasser, Adam J.; Kirkpatrick, J. Davy; Kuchner, Marc J.; Gramaize, Léopold; Rothermich, Austin; Brooks, Hunter; Vrba, Frederick J.; Bardalez Gagliuffi, Daniella; Caselden, Dan; Cushing, Michael C. (2021-11-01). "Ross 19B: An Extremely Cold Companion Discovered via the Backyard Worlds: Planet 9 Citizen Science Project". The Astrophysical Journal. 921 (2): 140. arXiv: 2108.05321. Bibcode: 2021ApJ...921..140S. doi: 10.3847/1538-4357/ac1c75. ISSN 0004-637X.
- ^ Ross, Frank E. (1925-11-01). "New proper-motion stars, (first list)". The Astronomical Journal. 36: 96–99. Bibcode: 1925AJ.....36...96R. doi: 10.1086/104687. ISSN 0004-6256.
- ^ "5118 Program Information". www.stsci.edu. Retrieved 2024-07-21.