TY - JOUR
T1 - NGTS clusters survey -- III
T2 - a low-mass eclipsing binary in the Blanco 1 open cluster spanning the fully convective boundary
AU - Smith, Gareth D.
AU - Gillen, Edward
AU - Queloz, Didier
AU - Hillenbrand, Lynne A.
AU - Acton, Jack S.
AU - Alves, Douglas R.
AU - Anderson, David R.
AU - Bayliss, Daniel
AU - Briegal, Joshua T.
AU - Burleigh, Matthew R.
AU - Casewell, Sarah L.
AU - Delrez, Laetitia
AU - Dransfield, Georgina
AU - Ducrot, Elsa
AU - Gill, Samuel
AU - Gillon, Michaël
AU - Goad, Michael R.
AU - Günther, Maximilian N.
AU - Henderson, Beth A.
AU - Jenkins, James S.
AU - Jehin, Emmanuël
AU - Moyano, Maximiliano
AU - Murray, Catriona A.
AU - Pedersen, Peter P.
AU - Sebastian, Daniel
AU - Thompson, Samantha
AU - Tilbrook, Rosanna H.
AU - Triaud, Amaury H. M. J.
AU - Vines, Jose I.
AU - Wheatley, Peter J.
PY - 2021/11
Y1 - 2021/11
N2 - We present the discovery and characterization of an eclipsing binary identified by the Next Generation Transit Survey in the ∼115-Myr-old Blanco 1 open cluster. NGTS J0002−29 comprises three M dwarfs: a short-period binary and a companion in a wider orbit. This system is the first well-characterized, low-mass eclipsing binary in Blanco 1. With a low mass ratio, a tertiary companion, and binary components that straddle the fully convective boundary, it is an important benchmark system, and one of only two well-characterized, low-mass eclipsing binaries at this age. We simultaneously model light curves from NGTS, TESS, SPECULOOS, and SAAO, radial velocities from VLT/UVES and Keck/HIRES, and the system’s spectral energy distribution. We find that the binary components travel on circular orbits around their common centre of mass in Porb = 1.098 005 24 ± 0.000 000 38 d, and have masses Mpri = 0.3978 ± 0.0033 M⊙ and Msec = 0.2245 ± 0.0018 M⊙, radii Rpri = 0.4037 ± 0.0048 R⊙ and Rsec = 0.2759 ± 0.0055 R⊙, and effective temperatures Tpri=3372+44−37 K and Tsec=3231+38−31 K. We compare these properties to the predictions of seven stellar evolution models, which typically imply an inflated primary. The system joins a list of 19 well-characterized, low-mass, sub-Gyr, stellar-mass eclipsing binaries, which constitute some of the strongest observational tests of stellar evolution theory at low masses and young ages.
AB - We present the discovery and characterization of an eclipsing binary identified by the Next Generation Transit Survey in the ∼115-Myr-old Blanco 1 open cluster. NGTS J0002−29 comprises three M dwarfs: a short-period binary and a companion in a wider orbit. This system is the first well-characterized, low-mass eclipsing binary in Blanco 1. With a low mass ratio, a tertiary companion, and binary components that straddle the fully convective boundary, it is an important benchmark system, and one of only two well-characterized, low-mass eclipsing binaries at this age. We simultaneously model light curves from NGTS, TESS, SPECULOOS, and SAAO, radial velocities from VLT/UVES and Keck/HIRES, and the system’s spectral energy distribution. We find that the binary components travel on circular orbits around their common centre of mass in Porb = 1.098 005 24 ± 0.000 000 38 d, and have masses Mpri = 0.3978 ± 0.0033 M⊙ and Msec = 0.2245 ± 0.0018 M⊙, radii Rpri = 0.4037 ± 0.0048 R⊙ and Rsec = 0.2759 ± 0.0055 R⊙, and effective temperatures Tpri=3372+44−37 K and Tsec=3231+38−31 K. We compare these properties to the predictions of seven stellar evolution models, which typically imply an inflated primary. The system joins a list of 19 well-characterized, low-mass, sub-Gyr, stellar-mass eclipsing binaries, which constitute some of the strongest observational tests of stellar evolution theory at low masses and young ages.
KW - binaries: eclipsing
KW - binaries: spectroscopic
KW - open clusters and associations: individual: Blanco 1
KW - stars: evolution
KW - stars: fundamental parameters
KW - stars: low mass
UR - http://www.scopus.com/inward/record.url?scp=85116980883&partnerID=8YFLogxK
U2 - 10.1093/mnras/stab2374
DO - 10.1093/mnras/stab2374
M3 - Article
SN - 0035-8711
VL - 507
SP - 5991
EP - 6011
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 4
ER -