Optical photometry of the eclipsing Large Magellanic Cloud supersoft source CAL87

被引:13
作者
Alcock, C
Allsman, RA
Alves, DR
Axelrod, TS
Bennett, DP
Charles, PA
Cook, KH
ODonoghue, D
Freeman, KC
Griest, K
Guern, J
Lehner, MJ
Livio, M
Marshall, SL
Minniti, D
Peterson, BA
Pratt, MR
Quinn, PJ
Rodgers, AW
Southwell, KA
Stubbs, CW
Sutherland, W
Welch, DL
机构
[1] UNIV CALIF BERKELEY,CTR PARTICLE ASTROPHYS,BERKELEY,CA 94720
[2] AUSTRALIAN NATL UNIV,SUPERCOMP FACIL,CANBERRA,ACT 0200,AUSTRALIA
[3] UNIV CALIF DAVIS,DEPT PHYS,DAVIS,CA 95616
[4] AUSTRALIAN NATL UNIV,MT STROMLO & SIDING SPRING OBSERV,WESTON,ACT 2611,AUSTRALIA
[5] UNIV OXFORD,DEPT ASTROPHYS,NUCL & ASTROPHYS LAB,OXFORD OX1 3RH,ENGLAND
[6] UNIV CAPE TOWN,DEPT ASTRON,ZA-7700 RONDEBOSCH,SOUTH AFRICA
[7] UNIV CALIF SAN DIEGO,DEPT PHYS,SAN DIEGO,CA 92093
[8] SPACE TELESCOPE SCI INST,BALTIMORE,MD 21218
[9] UNIV CALIF SANTA BARBARA,DEPT PHYS,SANTA BARBARA,CA 93106
[10] UNIV WASHINGTON,DEPT ASTRON,SEATTLE,WA 98195
[11] UNIV WASHINGTON,DEPT PHYS,SEATTLE,WA 98195
[12] MCMASTER UNIV,DEPT PHYS & ASTRON,HAMILTON,ON L8S 4M1,CANADA
基金
美国国家科学基金会;
关键词
accretion; accretion discs; binaries; close; spectroscopic; stars; individual; CAL87; Magellanic Clouds; X-rays;
D O I
10.1093/mnras/287.3.699
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present optical photometry of the eclipsing supersoft source CAL 87. These observations comprise long-term data accumulated as a by-product of the MACHO Project, and high-speed, white-light photometry of a single eclipse. We (i) derive an improved ephemeris of T-0 = HJD 245 0111.5144(3) + 0.442 677 14(6)E for the time of minimum light, (ii) find the eclipse structure to be stable over a period of similar to 4 yr, and (iii) investigate the colour variation as a function of orbital phase. The resolution afforded by the high-speed nature of the white-light observations enables us to see new structure in the light-curve morphology.
引用
收藏
页码:699 / 704
页数:6
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