discov_num |
notes |
refcode |
MCA 19 |
115 Tau. A is an occultation binary which has been resolved by |
|
|
speckle interferometry. |
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|
First detected as an occultation binary by Africano. |
Afr1978 |
|
1982.7551: All archival data for this system were reprocessed using |
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|
more powerful algorithms than earlier available, resulting in four new |
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|
unresolved measures as well as the new 1991 measurement. In addition, |
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|
new rho and theta values have been determined for the observations |
McA1989 |
|
originally published from 1986.9-1988.3 (McAlister et al. 1989), |
McA1990 |
|
1988.7-1989.2 (McAlister et al. 1990), and 1990.3--1990.8 (Hartkopf |
Hrt1992b |
|
et al. 1992). A preliminary orbit gives a period of ~15.3 years and |
|
|
a semi-major axis of 0".080. |
Hrt1994 |
|
1988.2518: This date was incorrectly given as 1988.2490 in McAlister |
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|
et al. (1989). |
McA1989 |
|
Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and |
|
|
spectroscopic masses 6.46 +/- 2.35, 8.01, and 4.79 Msun, respectively. |
Mlk2012 |
refcode |
metd |
author |
reference |
Afr1978 |
O j |
Africano, J.L., Evans, D., Fekel, F., Smith, B., & Morgan, C. |
1978AJ.....83.1100A |
Afr1978 |
|
AJ 83, 1100, 1978 |
|
Hrt1992b |
Sc j |
Hartkopf, W.I., McAlister, H.A., & Franz, O.G. |
1992AJ....104..810H |
Hrt1992b |
|
AJ 104, 810, 1992 |
|
Hrt1994 |
Sc j |
Hartkopf, W.I., McAlister,H.A., Mason, B.D., Barry, D.J., Turner, N., & Fu, H.-H. |
1994AJ....108.2299H |
Hrt1994 |
|
AJ 108, 2299, 1994 |
|
McA1989 |
Sc j |
McAlister, H.A., Hartkopf, W.I., Sowell, J.R., Dombrowski, E.G., & Franz, O.G. |
1989AJ.....97..510M |
McA1989 |
|
AJ 97, 510, 1989 |
|
McA1990 |
Sc j |
McAlister, H.A., Hartkopf, & Franz, O.G. |
1990AJ.....99..965M |
McA1990 |
|
AJ 99, 965, 1990 |
|
Mlk2012 |
not - |
Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. |
2012A&A...546A..69M |
Mlk2012 |
|
A&A 546, A69, 2012 |
|
Tok2020e |
St j |
Tokovinin, A., Mason, B.D., Mendez, R.A., Costa, E. & Horch, E.P. |
2020AJ....160....7T |
Tok2020e |
+orb |
AJ 160, 7, 2020 |
|