Published 1987
| Version v1
Miscellaneous
A high resolution study of diffuse interstellar bands
Creators
- 1. Uppsala Ionospheric Observatory (Sweden)
- 2. Institute of Astronomy, Torun (Poland)
Description
High resolution (0.05 A) spectra are used for the determination of the profiles of the diffuse interstellar bands 5780 and 5797 originating in single clouds. It is shown that some of the clouds may contain agents of certain diffuse bands whereas others may not. The profiles of diffuse bands observed in distant stars contain contributions from several clouds, differing in optical properties, which share the Doppler displacements observed in interstellar sodium lines. The Doppler splitting inside the diffuse bands' profiles is, however, efficiently veiled because of the large intrinsic widths of the bands under consideration. (author). 7 figs., 15 res
Additional details
Publishing Information
- Imprint Title
- Evolution of galaxies
- Imprint Pagination
- 479 p.
- Journal Page Range
- p. 231-235.
- Report number
- INIS-mf--11401
Conference
- Title
- 10. European regional astronomy meeting of the IAU.
- Dates
- 24-29 Aug 1987.
- Place
- Prague (Czechoslovakia).
INIS
- Country of Publication
- Serbia and Montenegro
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 20035919
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ABSORPTION SPECTRA; COSMIC DUST; COSMIC GASES; INTERSTELLAR SPACE
- Descriptors DEC
- DUSTS; FLUIDS; GASES; SPACE; SPECTRA