| discov_num |
notes |
refcode |
| STF2382 |
A: eps 1 Lyr = 4 Lyr |
|
|
AB: A premature orbit has been computed. |
|
| STFA 37 |
AB,CD: See ADS for notes of components. |
A__1932a |
|
AB and CD form the physical quadruple eps Lyrae, separation |
|
|
208". The observed small RV variations in each pair are probably |
|
|
merely scatter due to the very poor lines. |
|
|
BD: SHY 307. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
| STF2383 |
C: eps 2 Lyr = 5 Lyr |
|
| CHR 77 |
Ca: See note for 18323-1439 = CHR 73. |
Hrt1996b |
|
Ca is an Alpha CVn-type variable. |
|
|
The measures show a large scatter and there are many observations of |
|
|
the wider pair without a measure of this close companion. The nature |
|
|
of the motion or even the reality of this pair is in question. |
Tok2010b |
| STF2383 |
The longitude of periastron in the orbit of CD has been corrected. |
Gzl1956a |
| SHJ 277 |
EF, EG, etc.: A preliminary sketch of the motions of the SHJ group |
|
|
show the G component may be flying away in position angle ~190 |
Dal2002a |
| STF2382 |
AB: H 2 5. STF2383CD: H 2 6. |
MEv2010 |
| refcode |
metd |
author |
reference |
| A__1932a |
Ma - |
Aitken, R.G. |
1932QB821.A43...... |
| A__1932a |
|
Aitken Double Star Catalogue, 1932 |
|
| Dal2002a |
Ma u |
Daley, J.A. |
2002DSO.....8....1D |
| Dal2002a |
+C |
Double Star Observer 8, #1, 2002 |
|
| Gzl1956a |
orb - |
Guntzel-Lingner, U. |
1956AN....283...73G |
| Gzl1956a |
|
AN 283, 73, 1956 |
|
| Hrt1996b |
Sc j |
Hartkopf, W.I., Mason, B.D., McAlister, H.A., Turner, N.H., Barry, D.J., Franz, . |
1996AJ....111..936H |
| Hrt1996b |
|
O.G., & Prieto, C.M |
|
| Hrt1996b |
|
AJ 111, 936, 1996 |
|
| 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.) |
|
| Tok2010b |
S - |
Tokovinin, A. |
................... |
| Tok2010b |
|
private communication |
|
