Published January 1982
| Version v1
Journal article
Correlation between the age of a stellar aggregate and the color parameters of its member flare stars
Description
An empirical relation is established between the mean departure from the main sequence in the two-color (U-B, B-V) diagram (along the U-B axis) of a system of flare stars or Hα emission stars and the age of the aggregate containing that system (or of the nonstable stars belonging to the aggregate). The ages of four T Tau stars are estimated
Additional details
Publishing Information
- Journal Title
- Sov. Astron. Lett. (Engl. Transl.)
- Journal Volume
- 8
- Journal Issue
- 1
- Series
- Sov. Astron. Lett. (Engl. Transl.).
- Journal Page Range
- 19-22
- ISSN
- 0360-0327
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14790316
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AGE ESTIMATION; BALMER LINES; COLOR; ERUPTIVE VARIABLE STARS; PHOTOMETRY; STAR CLUSTERS; STAR EVOLUTION; T TAURI STARS
- Descriptors DEC
- OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; STARS; VARIABLE STARS
Optional Information
- Notes
- Cover-to-cover translation of Pis'ma v Astronomicheskij Zhurnal (USSR).