discov_num |
notes |
refcode |
DAE 9 |
WSP 12. WASP-12. Bergfors et al (2013) estimate spectral types G0V |
Brg2013 |
|
and K0-M0V. WASP-12b is one of the largest and hottest transiting |
|
|
planets; period 1.09d. Bergfors 6 is a point source ~3 mags fainter, |
|
|
at a separation of 1". Based on color, the companion is an M0-M1 main- |
|
|
sequence star. Relative photometry suggests Bergfors 6 is ~50% closer |
|
|
to Earth than is WASP-12, and that their consistent radial velocities |
|
|
are coincidental. If Bergfors 6 is a binary M dwarf system near |
|
|
conjunction, however, it could lie at a similar distance to WASP-12 |
|
|
and the system could be gravitationally bound. |
Csf2012 |
BEC 1 |
BC: Bechter et al. (2014) resolved the 1" companion to WASP 12 into 2 |
|
|
~equal magnitude stars, separated by 84 mas. Both components appear to |
|
|
be physically associated with the primary. Spectral types of B and C |
|
|
components M3V, masses 0.38 +/- 0.05 and 0.37 +/- 0.05 Msun. |
Bec2014 |
refcode |
metd |
author |
reference |
Bec2014 |
A j |
Bechter, E.B., Crepp, J.R., Ngo, H., Knutson, H.A., Batygin, K., Hinkley, S., |
2014ApJ...788....2B |
Bec2014 |
|
Muirhead, P.S., Johnson, J.A., Howard, A.W., Montet, B.T., Matthews, C.T., & |
|
Bec2014 |
|
Morton, T.D. |
|
Bec2014 |
|
ApJ 788, 2, 2014 |
|
Bec2014 |
|
(Their B and C component relabelled as Ba and Bb. Measures for close pairs |
|
Bec2014 |
|
generated from their A,Ba and A,Bb data) |
|
Brg2013 |
Cl j |
Bergfors, C. Brandner, W., Daemgen, S., Biller, B., Hippler, S., Janson, M., |
2013MNRAS.428..182B |
Brg2013 |
|
Kudryavtseva, N., Geissler, K., Henning, T., & Koehler, R. |
|
Brg2013 |
|
MNRAS 428, 182, 2013 |
|
Csf2012 |
H+ j |
Crossfield, I.J.M., Barman, T., Hansen, B.M.S., Tanaka, I., & Kodama, T. |
2012ApJ...760..140C |
Csf2012 |
+Ci |
ApJ 760, 140, 2012 |
|
idgroup |
discov |
author |
1 |
DAE |
Daemgen, S., Siegler, N., Reid, I.N., & Close, L.M. |
2 |
DAE |
Daemgen, S., Hormuth, F., Brandner, W., Bergfors, C., Janson, M., Hippler, S., & |
2 |
DAE |
Henning, T. |
5 |
DAE |
Daemgen, S., Petr-Gotzens, M.G., Correia, S., Teixeira, P.S., Brandner, W., |
5 |
DAE |
Kley, W., & Zinnecker, H. |