Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-10-20
Mon.Not.Roy.Astron.Soc. 349 (2004) 1059
Astronomy and Astrophysics
Astrophysics
15 pages, 9 figures (7 in low resolution), submitted to MNRAS. Article in full resolution can be obtained at http://www.astr
Scientific paper
10.1111/j.1365-2966.2004.07587.x
Among over 200,000 Galactic Bulge variable stars in the public domain OGLE catalogue, we found over 15,000 red giant variables following two well defined period -- amplitude relations. The periods are in the range 10 < P < 100 days, and amplitudes in the range 0.005 < A < 0.13 mag in I-band. The variables cover a broad range of reddening corrected colours, 1 < (V-I)_0 < 5, and a fairly narrow range of extinction corrected apparent magnitudes, 10.5 < I_0 < 13 . A subset of variables (type A) has a rms scatter of only 0.44 mag. The average magnitudes for these stars are well correlated with the Galactic longitude, and vary from I_{k,0} = 11.82 for l = +8 deg to I_{k,0} = 12.07 for l = -5 deg, clearly indicating that they are located in the Galactic Bar. Most variables have several oscillation periods.
Eyer Laurent
Paczyński Bohdan
Wray James J.
No associations
LandOfFree
OGLE small amplitude red giant variables in the Galactic Bar 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 OGLE small amplitude red giant variables in the Galactic Bar, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OGLE small amplitude red giant variables in the Galactic Bar will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-509370