Published March 1976
| Version v1
Journal article
Scanner observations of M-type Mira variables
Creators
- 1. Tokyo Univ., Mitaka (Japan). Tokyo Astronomical Observatory
Description
The energy distribution in the range lambda lambda 3700-5500A was observed for several Mira variables of M-type. It is shown that the distribution of radiative fluxes measured at several flux peaks is an indicator of the intensities of TiO bands rather than an indicator of temperature. A brief discussion considers the possible correlation between the so-called general line weakening in Mira variables and an enhanced TiO opacity. (auth.)
Additional details
Identifiers
Publishing Information
- Journal Title
- Publications of the Astronomical Society of Japan
- Journal Volume
- 28
- Journal Issue
- 1
- Series
- Publ. Astron. Soc. Jpn.
- Journal Page Range
- 135-140
- ISSN
- 2053-051X
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 8294536
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ENERGY SPECTRA; OPACITY; SPECTROPHOTOMETRY; VARIABLE STARS; VISIBLE RADIATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SPECTRA; STARS
Optional Information
- Notes
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