Published 1989
| Version v1
Journal article
Period variability of the detached eclipsing binary system TX Her
Creators
- 1. Wyzsza Szkola Pedagogiczna, Cracow (Poland)
- 2. Uniwersytet Jagiellonski, Cracow (Poland). Obserwatorium Astronomiczne
Description
The behaviour of O-C changes for the TX Her system based on the list of primary minima moments available in the literature, together with the three ones obtained by us is discussed. Assuming the changes are due to a ''third body'' rotating around the TX Her system, the parameters of the third body's orbit are determined. The mass of the third component should be not less than 0.46 solar masses. 37 refs., 2 figs., 3 tabs. (author)
Additional details
Publishing Information
- Journal Title
- Acta Astronomica
- Journal Volume
- 39
- Journal Issue
- 3
- Series
- Acta Astron.
- Journal Page Range
- 243-249
- ISSN
- 0001-5237
- CODEN
- AASWA
INIS
- Country of Publication
- Poland
- Country of Input or Organization
- Poland
- INIS RN
- 22082479
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BINARY STARS; ECLIPSE; EXPERIMENTAL DATA; MASS; ORBITS; STARS; THEORETICAL DATA; VARIATIONS
- Descriptors DEC
- DATA; INFORMATION; NUMERICAL DATA