discov_num | notes | refcode |
KUI 41 | Ross 440. The primary is probably a flare star. | |
Pair often unresolved, so orbit probably eccentric with P<10y. | Kui1943 | |
See Baize & Petit (1989) catalog of doubles with variable component. | Baz1989d | |
Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | ||
masses of 0.74 +/- 0.21, 0.80, and 0.30 Msun, respectively. | Mlk2012 |
refcode | metd | author | reference |
Baz1989d | - | Baize, P. & Petit, M. | 1989A&AS...77..497B |
Baz1989d | A&AS 77, 497, 1989 | ||
Kui1943 | Mb - | Kuiper, G.P. | 1943ApJ....97..275K |
Kui1943 | ApJ 97, 275, 1943 | ||
Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
Mlk2012 | A&A 546, A69, 2012 | ||
MnA2019 | C j | Mann, A.W., Dupuy, T., Kraus, A.L., Gaidos, E., Ansdell, M., Ireland, M., Rizzuto, | 2019ApJ...871...63M |
MnA2019 | +orb | A.C., Hung, C..-L., Dittmann, J., Factor, S., Feiden, G., Martinez, R.A., | |
MnA2019 | Ruiz-Rodriguez, D. & Chia Thao, P. | ||
MnA2019 | ApJ 871, 63, 2019 |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
09313-1329 | KUI 41 | 1996 | 14 | 265 | 0.6 | 10.74 | 10.94 | dM4 | NOD | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2010 | 15 | 319 | 0.7 | 10.74 | 10.94 | dM4 | NOD | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2013 | 18 | 279 | 0.7 | 10.74 | 10.94 | dM4 | NOD | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2014 | 21 | 266 | 0.7 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2015 | 22 | 247 | 0.7 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2017 | 26 | 228 | 0.6 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2018 | 27 | 214 | 0.5 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2019 | 28 | 187 | 0.4 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 | |
09313-1329 | KUI 41 | 2020 | 29 | 103 | 0.4 | 10.74 | 10.94 | dM4 | NO | 093119.43-132919.3 |