Variable Stars in the Open Cluster NGC 7044
G. Kopacki, D. Drobek, Z. Kolaczkowski, G. Polubek

TL;DR
This study identifies and classifies 23 variable stars in the open cluster NGC 7044, including pulsating, eclipsing, and irregular variables, and estimates the cluster's distance, reddening, and age through photometric analysis.
Contribution
First comprehensive survey of variable stars in NGC 7044, including membership assessment and cluster parameter determination using photometric and period-luminosity relations.
Findings
23 variable stars identified in NGC 7044
Cluster distance modulus estimated at 14.2 mag
Derived cluster age of approximately 1.6 billion years
Abstract
We present results of a search for variable stars in the intermediate-age open cluster NGC 7044. We found 23 variable stars in the observed field. One star turned out to be of the delta Sct type with two pulsational modes excited. From the position in the color-magnitude diagram we conclude that this star is a member of the cluster. Moreover, we found 13 eclipsing systems, of which five are W UMa stars, one is a beta Lyr variable, six are beta Per binaries showing detached configuration, and the last one is another probable beta Per system. Using the period-luminosity-color relation for W UMa stars we established the membership of the contact binaries, finding four of them to be very probable cluster members. We estimated from these four stars an apparent distance modulus (m-M)_V of NGC 7044 to be 14.2 +/- 0.4 mag, which is smaller than previous determinations of this parameter. We were…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
