discov_num | notes | refcode |
HU 462 | 1997.1231: Our reduction does not give the quadrant unambiguously. We | |
therefore adopt the quadrant consistent with the latest measure in the | ||
WDS. | Hor1997 | |
Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | ||
masses of 1.65 +/- 0.25, 1.85, and 0.91 Msun, respectively. | Mlk2012 |
refcode | metd | author | reference |
Hor1997 | S j | Horch, E.P., Ninkov, Z., & Slawson, R. | 1997AJ....114.2117H |
Hor1997 | AJ 114, 2117, 1997 | ||
Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
Mlk2012 | A&A 546, A69, 2012 | ||
Msn2021c | orb - | Josties, J. & Mason, B.D. | 2021IAUDS.205....1M |
Msn2021c | Inf. Circ. 205, 1, 2021 |
idgroup | discov | author |
1 | HU | Hussey, W.F. |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
11272-1539 | HU 462 | 2005 | 88 | 165 | 0.4 | 8.42 | 8.53 | G8V | NOD | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2009 | 90 | 134 | 0.4 | 8.42 | 8.53 | G8V | NOD | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2010 | 94 | 134 | 0.4 | 8.42 | 8.53 | G8V | NOD | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2011 | 95 | 118 | 0.4 | 8.42 | 8.53 | G8V | NOD | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2013 | 96 | 97 | 0.4 | 8.42 | 8.53 | G8V | NOD | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2014 | 96 | 92 | 0.4 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2016 | 97 | 69 | 0.4 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2018 | 100 | 50 | 0.4 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2019 | 101 | 41 | 0.5 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2020 | 102 | 41 | 0.5 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 | |
11272-1539 | HU 462 | 2021 | 103 | 35 | 0.5 | 8.42 | 8.53 | G8V | NO | 112710.78-153855.0 |