TY - JOUR
T1 - Ross 19B
T2 - An Extremely Cold Companion Discovered via the Backyard Worlds: Planet 9 Citizen Science Project
AU - Schneider, Adam C.
AU - Meisner, Aaron M.
AU - Gagné, Jonathan
AU - Faherty, Jacqueline K.
AU - Marocco, Federico
AU - Burgasser, Adam J.
AU - Kirkpatrick, J. Davy
AU - Kuchner, Marc J.
AU - Gramaize, Léopold
AU - Rothermich, Austin
AU - Brooks, Hunter
AU - Vrba, Frederick J.
AU - Bardalez Gagliuffi, Daniella
AU - Caselden, Dan
AU - Cushing, Michael C.
AU - Gelino, Christopher R.
AU - Line, Michael R.
AU - Casewell, Sarah L.
AU - Debes, John H.
AU - Aganze, Christian
AU - Ayala, Andrew
AU - Gerasimov, Roman
AU - Gonzales, Eileen C.
AU - Hsu, Chih Chun
AU - Kiman, Rocio
AU - Popinchalk, Mark
AU - Theissen, Christopher
N1 - Publisher Copyright:
© 2021. The American Astronomical Society. All rights reserved.
PY - 2021/11/10
Y1 - 2021/11/10
N2 - Through the Backyard Worlds: Planet 9 citizen science project, we have identified a wide-separation (∼10′, ∼9900 au projected) substellar companion to the nearby (∼17.5 pc), mid-M dwarf Ross 19. We have developed a new formalism for determining chance alignment probabilities based on the BANYAN Σ tool, and find a 100% probability that this is a physically associated pair. Through a detailed examination of Ross 19A, we find that the system is metal-poor ([Fe/H] = -0.40 ± 0.12) with an age of 7.2-3.6+3.8 Gyr. Combining new and existing photometry and astrometry, we find that Ross 19B is one of the coldest known wide-separation companions, with a spectral type on the T/Y boundary, an effective temperature of 500-100+115 K, and a mass in the range 15-40 M Jup. This new, extremely cold benchmark companion is a compelling target for detailed characterization with future spectroscopic observations using facilities such as the Hubble Space Telescope or James Webb Space Telescope.
AB - Through the Backyard Worlds: Planet 9 citizen science project, we have identified a wide-separation (∼10′, ∼9900 au projected) substellar companion to the nearby (∼17.5 pc), mid-M dwarf Ross 19. We have developed a new formalism for determining chance alignment probabilities based on the BANYAN Σ tool, and find a 100% probability that this is a physically associated pair. Through a detailed examination of Ross 19A, we find that the system is metal-poor ([Fe/H] = -0.40 ± 0.12) with an age of 7.2-3.6+3.8 Gyr. Combining new and existing photometry and astrometry, we find that Ross 19B is one of the coldest known wide-separation companions, with a spectral type on the T/Y boundary, an effective temperature of 500-100+115 K, and a mass in the range 15-40 M Jup. This new, extremely cold benchmark companion is a compelling target for detailed characterization with future spectroscopic observations using facilities such as the Hubble Space Telescope or James Webb Space Telescope.
UR - http://www.scopus.com/inward/record.url?scp=85120628486&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85120628486&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ac1c75
DO - 10.3847/1538-4357/ac1c75
M3 - Article
AN - SCOPUS:85120628486
SN - 0004-637X
VL - 921
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 140
ER -