F. Jablonski, J. E. Steiner
Abstract
The authors report the discovery of an ultrashort binary period in the star NSV 12615 ≡ S7273. The object shows deep eclipses (Δm ≈ 1.2) and has a period of 88.45 minutes. It is suggested that the star belongs to the SU UMa subclass of dwarf novae.
OpenAlex reports 5 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The authors report the discovery of an ultrashort binary period in the star NSV 12615 ≡ S7273. The object shows deep eclipses (Δm ≈ 1.2) and has a period of 88.45 minutes. It is suggested that the star belongs to the SU UMa subclass of dwarf novae.
Key concepts: Physics, Astrophysics, Cataclysmic variable star, Stars, Light curve, Binary star, Variable star, Astronomy