2006AJ....131.3028Q


Query : 2006AJ....131.3028Q

2006AJ....131.3028Q - Astron. J., 131, 3028-3039 (2006/June-0)

Deep, low mass ratio overcontact binary systems. VI. AH Cancri in the old open cluster M67.

QIAN S.-B., LIU L., SOONTHORNTHUM B., ZHU L.-Y. and HE J.-J.

Abstract (from CDS):

CCD photometric light curves in the B and V bands obtained in 2001 and in the V band obtained in 2002 of AH Cnc in the old open cluster M67 are presented. It is shown that AH Cnc is a total-eclipsing binary and its light curves correspond to a typical A type according to Binnendijk's classification. The variations of the light curve around the primary minimum and second maximum were found. Our nine epochs of light minimum monitored from 2001 to 2005, including others collected from the literature, were used to create the first study of the period changes of the binary system. A cyclic oscillation with a period of 36.5 yr and an amplitude of 0.0237 days was discovered to be superposed on a continuous period increase (dP/dt=3.99x10–7 days/yr). Weak evidence indicates that there exists another small-amplitude period oscillation (A4=0.0035 days, P4=7.75 yr). The symmetric light curves in the B and V bands obtained in 2001 were analyzed with the 2003 version of the Wilson-Devinney code. It is confirmed that AH Cnc is a deep overcontact binary system with a high degree of overcontact f=58.5%±4.5% and a low mass ratio of q=0.1682±0.0012. The existence of the third light and the cyclic period oscillation both may suggest that AH Cnc is a triple system containing an unseen third body. The tertiary component may have played an important role in the origin of the overcontact binary star by removing angular momentum from the central system, which would cause it to have a short initial orbital period and thus evolve into an overcontact configuration by angular momentum loss. The long-term period increase can be interpreted as a mass transfer from the less massive component to the more massive one. As the orbital period increases, the decrease of the mass ratio will cause it finally to evolve into a single rapid-rotating star when the system meets the more familiar criterion that the orbital angular momentum be less than 3 times the total spin angular momentum. Therefore, AH Cnc may be a progenitor of the blue straggler stars in M67.

Abstract Copyright: ∼

Journal keyword(s): Stars: Binaries: Close - Stars: Binaries: Eclipsing - Galaxy: Open Clusters and Associations: Individual: Messier Number: M67 - Stars: Evolution - stars: individual (AH Cnc)

Simbad objects: 24

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Number of rows : 24
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 V* CU Tau EB* 03 47 36.9103738080 +25 23 15.845178660   12.02 11.23 11.38 10.678 G0 66 0
2 V* YY Eri SB* 04 12 08.8493445840 -10 28 09.993826452   9.08 8.41   7.673 G3V 226 0
3 V* IK Per EB* 04 29 27.4573781040 +42 03 10.585181376   12.17 11.49     A2 59 0
4 HD 280332A SB* 05 01 10.8328702632 +34 30 26.555760288   10.94 10.34     ~ 110 0
5 HD 280332 ** 05 01 10.83934 +34 30 26.5819   10.901 10.215 10.047 9.305 G0 97 0
6 V* ER Ori SB* 05 11 14.5056264672 -08 33 24.613510680   10.02 9.46 8.927 8.604 F7/8V 187 0
7 V* FG Hya SB* 08 27 03.9412969584 +03 30 52.329583548   10.62 10.04 9.544 9.401 G0 213 0
8 NGC 2682 55 BS* 08 51 03.5144925000 +11 45 02.822542776   11.61 11.295   10.941 B9V 77 0
9 NGC 2682 OpC 08 51 23.5 +11 48 54           ~ 2528 0
10 NGC 2682 153 BS* 08 51 26.4321697248 +11 43 50.738037528   11.41 11.269   11.101 A2V 95 0
11 NGC 2682 185 BS* 08 51 32.5946133024 +11 48 52.103681712   11.46 11.48   10.80 A0V 75 0
12 Cl* NGC 2682 SAND 1282 SB* 08 51 37.8473566296 +11 50 57.092451072 13.964 13.89 13.333   12.634 F7V 181 0
13 V* XY Leo ** 10 01 40.4170488672 +17 24 32.602180644   10.66 9.68 8.855 8.474 K0V 287 0
14 V* AW UMa SB* 11 30 04.3160006304 +29 57 52.674404544   7.27   6.7   F0 302 0
15 V* TV Mus EB* 11 39 57.7633052952 -64 48 59.229170568   11.48 10.75   9.712 F2 76 0
16 V* CE Leo EB* 11 44 24.2554757472 +23 21 22.849119288   12.602 12.39 11.27 10.798 K 93 0
17 V* XY Boo SB* 13 49 11.5666861776 +20 11 24.590393088   10.71 10.54 9.994 9.698 F5V 154 0
18 V* CK Boo SB* 14 35 03.7596377832 +09 06 49.373523360   9.61 9.029 8.683 8.414 F7/8V 150 0
19 V* GR Vir SB* 14 45 20.2632619872 -06 44 04.131471300   8.54 8.00   7.34 G2/3V 151 0
20 V* V857 Her SB* 16 46 53.5600592376 +38 38 58.246857528   11.04 10.87 9.808 9.558 A6 96 1
21 V* AK Her SB* 17 13 57.8236051704 +16 21 00.618202044   9.04 8.51   7.874 F4V 271 0
22 V* V839 Oph SB* 18 09 21.2653435464 +09 09 03.607091388   9.62 9.03   8.286 F7V 147 0
23 V* V417 Aql SB* 19 35 24.1195136928 +05 50 17.661574140   11.23 10.63 10.629 10.276 G0V+F9V 131 0
24 V* BX Peg EB* 21 38 49.3910800824 +26 41 34.213405092     10.890     G4.5 142 0

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