1992IAUS..151..473M


Query : 1992IAUS..151..473M

1992IAUS..151..473M - 151th Symposium of the IAU, held in Cordoba, Argentina, August 5-9 1991. Ed. by Y. Kondo, R.F. Sistero and R.S. Polidan. "Evolutionary Processes in interacting binary stars"., 151, 473-474 (1992)

Can evolution in close binaries account for the blue stargglers in M 67 ?

MILONE A.A.E., LATHAM D.W., MATHIEU R.D., MORSE J.A. and DAVIS R.J.

Journal keyword(s):

Simbad objects: 14

goto View the references in ADS

Number of rows : 14
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 2682 55 BS* 08 51 03.5144925000 +11 45 02.822542776   11.61 11.295   10.941 B9V 77 0
2 NGC 2682 81 BS* 08 51 11.7789373696 +11 45 22.123673277   9.96 10.024     B8V 114 0
3 NGC 2682 90 BS* 08 51 14.3529693120 +11 45 00.540874080   11.43 10.819   10.544 ~ 51 0
4 NGC 2682 124 BS* 08 51 19.9070240880 +11 47 00.441178944 12.576 12.59 12.117 11.848 11.564 F5IV 90 0
5 NGC 2682 131 SB* 08 51 20.794032 +11 53 26.13120   11.647 11.248 11.042 10.722 F5IV 128 0
6 NGC 2682 OpC 08 51 23.5 +11 48 54           ~ 2528 0
7 NGC 2682 153 BS* 08 51 26.4321697248 +11 43 50.738037528   11.41 11.269   11.101 A2V 95 0
8 NGC 2682 156 BS* 08 51 27.0120114864 +11 51 52.582244112   11.1 10.940   10.862 A2V 81 0
9 Cl* NGC 2682 SAND 1280 dS* 08 51 32.5773312840 +11 50 40.634470500 12.537 12.52 12.269 12.121 11.922 F0 67 0
10 NGC 2682 185 BS* 08 51 32.5946133024 +11 48 52.103681712   11.46 11.48   10.80 A0V 75 0
11 Cl* NGC 2682 SAND 1284 BS* 08 51 34.3150275672 +11 51 10.497400452   11.17 10.92   10.622 B9V 106 0
12 NGC 2682 207 BS* 08 51 37.6915341325 +11 37 03.761045440 12.629 12.91 12.344   11.777 F2V 40 0
13 NGC 2682 238 BS* 08 51 48.6395454552 +11 49 15.654839376   11.23 10.913     A1V 55 0
14 BD+12 1930 BS* 08 52 10.7435074328 +11 44 05.867673842   10.81 10.700     A1V 71 0

To bookmark this query, right click on this link: simbad:objects in 1992IAUS..151..473M and select 'bookmark this link' or equivalent in the popup menu