Published January 15, 1975
| Version v1
Journal article
The composite spectrum and energy distribution of XX Ophiuchi
Description
Broad-band photometry from 0.36 to 10.2 , narrow-band photometry and scans from 0.75 to 1.08 iL and Fourier transform spectrometry from 1.4 to 2.3 show that the peculiar Be star XX Oph has a cool companion with a spectral type of M6. The observed energy distribution can be represented by a BO III star and an M6 III star reddened by 4 mag of visual extinction. Subject headings: Be stars - binaries - spectrophotometry - stars, individual
Additional details
Identifiers
- DOI
- 10.1086/153336;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 195
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 385
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6188927
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; ENERGY SPECTRA; HYDROGEN; INFRARED RADIATION; METALS; SPECTROPHOTOMETRY
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTS; NONMETALS; RADIATIONS; SPECTRA; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent