New variable stars in Sgr B (Terzan+, 1982)

Details New variable stars in Sgr B (Terzan+, 1982) New variable stars in Sgr B (Terzan+, 1982)

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ycat..40490715t&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/49/715. Originally published in: 1982A&AS...49..715T

Astronomy and Astrophysics

Astronomy

Stars: Variable, Photometry: Photographic

Scientific paper

621 new variable stars have been detected on plates obtained with the Schmidt telescopes of the Mount Palomar Observatory (1968) and of the European Southern Observatory (1976-1980). The astrometric measurements (ESO-CERN) and the photometrical ones (CDCA) which have followed the detection the variable stars (Observatoire de Lyon) have led to determine the parameters α, δ, l, b, R(Max), R(Min), δm. So we notice that: - 379 variable stars have an amplitude of variation in magnitude between 0.5 and 2.0 (delm/N histogram). -The number of variable stars strongly decreases towards the great amplitudes. -The surface density of variable stars by square degree in this central galactic direction increases from 2 to 21 in the explored field of 5.5degx5.5deg size. (2 data files).

Affiliated with

Also associated with

No associations

Rating

New variable stars in Sgr B (Terzan+, 1982) 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 New variable stars in Sgr B (Terzan+, 1982), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New variable stars in Sgr B (Terzan+, 1982) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950851