discov_num |
notes |
refcode |
STTA 45 |
AB: H VI 98. A is V774 Tau. B is BD+05@613, and a suspected variable. |
|
|
AB: SHY 21. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
|
AB: H 6 98. |
MEv2010 |
|
Toyota et al. (2009) monitored the RV of both the A and B components |
|
|
every 1-2 months between 2003 Mar - 2007 Nov, using a high-dispersion |
|
|
echelle (precision ~10 m/s). Standard deviations of the RVs of both |
|
|
components are <40 m/s and velocities show no periodic variation. |
|
|
These results rejects the association of a planet of mass > 1.8 Mjup |
|
|
with either star. |
Toy2009 |
refcode |
metd |
author |
reference |
MEv2010 |
- |
MacEvoy, B. |
................... |
MEv2010 |
|
private communication, 2010 (see http://www.handprint.com/ASTRO/index.html) |
|
Shy2011 |
- |
Shaya, E.J. & Olling, R. |
2011ApJS..192....2S |
Shy2011 |
|
ApJS 192, 2, 2011 |
|
Shy2011 |
|
(Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs |
|
Shy2011 |
|
added to WDS only if probability 90% or greater.) |
|
Toy2009 |
rv - |
Toyota, E., Itoh, Y., Ishiguma, S., Urakawa, S., Murata, D., Oasa, Y., |
2008PASJ...61...19T |
Toy2009 |
|
Matsuyama, H., Funayama, H., Sato, B., & Mukai, T. |
|
Toy2009 |
|
PASJ 61, 19, 2009 |
|