| discov_num |
notes |
refcode |
| STF 738 |
lam Ori = Meissa |
|
|
Both A and B components were observed and appeared to be single. The |
|
|
AB pair may not be physical (Lindroos). The photometry-based |
Lnd1985 |
|
classification of the C component is from Lindroos, who also gives a |
|
|
distance of 430 pc. |
Msn1998a |
|
Classification of the B component is from Hoffleit & Warren (1991). |
Hof1991 |
|
AB: The image rotator was in an unknown state, so two possible theta |
|
|
values are listed for the 2001.7428 observation - one for zenith up |
|
|
and one for north up. |
Trn2008 |
|
AB: H 2 9. |
MEv2010 |
|
Uniform disk diameter 0.219 +/- 0.015 mas, |
|
|
Limb darkened diameter 0.228 +/- 0.009 mas, |
|
|
Teff = 36,000 +/- 900 K, Radius is 10.2 +/- 1.3 \rsun. |
CIA2018e |
| refcode |
metd |
author |
reference |
| CIA2018e |
not j |
Gordon, K.D., Gies, D.R., Schaefer, G.H., Huber, D., Ireland, M. & Hillier, D.J. |
2018ApJ...869...37G |
| CIA2018e |
|
ApJ 869, 37, 2018 |
|
| Hof1991 |
- |
Hoffleit, D. & Jaschek, C. |
1991bsc..book.....H |
| Hof1991 |
|
The Bright Star Catalogue, Fifth Revised Edition (preliminary version), 1991 |
|
| Lnd1985 |
- |
Lindroos, K.P. |
1985A&AS...60..183L |
| Lnd1985 |
|
A&AS 60, 183, 1985 |
|
| MEv2010 |
- |
MacEvoy, B. |
................... |
| MEv2010 |
|
private communication, 2010 (see http://www.handprint.com/ASTRO/index.html) |
|
| Msn1998a |
Sc j |
Mason, B.D., Gies, D.R., Hartkopf, W.I., Bagnuolo, Jr., W.G., |
1998AJ....115..821M |
| Msn1998a |
|
ten Brummelaar, T.A., & McAlister, H.A. |
|
| Msn1998a |
|
AJ 115, 821, 1998 |
|
| Trn2008 |
Ac j |
Turner, N.H., ten Brummelaar, T.A., Roberts, L.C., Mason, B.D., Hartkopf, W.I., & |
2008AJ....136..554T |
| Trn2008 |
+E2 |
Gies, D.R. |
|
| Trn2008 |
+A |
AJ 136, 554, 2008 |
|
| Trn2008 |
|
(Note: For some observations the image derotator was in an unknown state. In these |
|
| Trn2008 |
|
cases the theta value is either left blank or two possible values are listed - one |
|
| Trn2008 |
|
for zenith up and one for north up. For unresolved objects, the listed rho value |
|
| Trn2008 |
|
is the FWHM of the corrected stellar PSF. Larger FWHM values are indicative of |
|
| Trn2008 |
|
poorer seeing and/or non-optimal AO system tuning.) |
|
