Light curves of the PMS system TY CrA (Vaz+ 1998)

Details Light curves of the PMS system TY CrA (Vaz+ 1998) Light curves of the PMS system TY CrA (Vaz+ 1998)

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..41300245v&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/130/245. Originally published in: 1998A&AS..130..245V

Physics

Binaries: Eclipsing, Photometry: Uvby

Scientific paper

Complete uvby light curves of the detached Herbig Be eclipsing binary TY Coronae Australis are presented. A total of 1787 photometric measurements in each of the four colours were obtained in 1989 and in 1992-1994. A detailed analysis of the y light curve obtained in 1992-1993 is published separately (Casey et al. 1997). The reflection nebula around the system contributes about 30% of the light in all four passbands. Here we present and discuss the non-eclipse-related photometric variability of the system. We suggest that these variations are the result of variable obscuration, possibly linked to dust shells physically associated to the system. (1 data file).

Affiliated with

Also associated with

No associations

Rating

Light curves of the PMS system TY CrA (Vaz+ 1998) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Light curves of the PMS system TY CrA (Vaz+ 1998), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light curves of the PMS system TY CrA (Vaz+ 1998) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-926806