SIMULTANEOUS OPTICAL AND IR PHOTOMETRY OF THE T-TAURI STAR RU LUPI

被引:0
作者
GIOVANNELLI, F
ERRICO, L
VITTONE, AA
ROSSI, C
机构
[1] OSSERV ASTRON CAPODIMONTE,VIA MOIARIELLO 16,I-80131 NAPLES,ITALY
[2] CNR,IST ASTROFIS SPAZIALE,I-00044 FRASCATI,ITALY
[3] UNIV ROME,INST ASTRON,I-00185 ROME,ITALY
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1991年 / 87卷 / 01期
关键词
STARS; PHOTOMETRY; PRE-MAIN-SEQUENCE; ROTATION OF; RU LUPI;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Two simultaneous optical and IR photometric observation runs of RU Lupi were carried out at the European Southern Observatory (ESO) in February 1983 and in June 1986 within the framework of a large multifrequency coordinated campaign of observations. RU Lupi was found in two different states. In the first case the star was in "quiescence", in the second it was brighter and showed larger variations due to a flare like event (FLE). A positive correlation between luminosity and its variations has been found. A Fourier analysis of the light curve available in literature was performed to point out the rotational period. The analysis of these data excludes any periodicity. Our colour-colour diagnostic diagram clearly shows that RU Lupi variability is mainly due to a strong photospheric an chromospheric activity.
引用
收藏
页码:89 / 95
页数:7
相关论文
共 27 条
  • [1] [Anonymous], S AFR ASTR OBS CIRC
  • [2] [Anonymous], VEROEFFENTLICHUNGEN
  • [3] Appenzeller I., 1983, Astronomy & Astrophysics Supplement Series, V53, P291
  • [4] Bastian U., 1979, Astronomy and Astrophysics Supplement Series, V36, P57
  • [5] Bisnovatyi-Kogan G. S., 1977, Soviet Astronomy, V21, P720
  • [6] BISNOVATYIKOGAN GS, 1980, SVA LETT, V6, P17
  • [7] HIGH-RESOLUTION SPECTROSCOPY OF THE T-TAURI STAR RU LUPI
    BOESGAARD, AM
    [J]. ASTRONOMICAL JOURNAL, 1984, 89 (11) : 1635 - &
  • [8] EVANS A, 1981, ASTROPHYS SPACE SIC, V74, P2325
  • [9] T-TAURI STAR RU LUPI AND ITS CIRCUMSTELLAR SURROUNDING
    GAHM, GF
    NORDH, HL
    OLOFSSON, SG
    [J]. ICARUS, 1975, 24 (03) : 372 - 378
  • [10] GAHM GF, 1974, ASTRON ASTROPHYS, V33, P399