Three components of 3?4 ?m absorption bands
- 1 December 1983
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 97 (2) , 369-378
- https://doi.org/10.1007/bf00653492
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Identification of the emission feature near 3.5 microns in the pre-main-sequence star HD 97048The Astrophysical Journal, 1983
- The variable infrared source near HH100Monthly Notices of the Royal Astronomical Society, 1982
- Diffuse interstellar absorption bands between 2.9 and 4.0 µmNature, 1981
- Observations of unidentified infrared features in the pre-main sequence star HD 97048Monthly Notices of the Royal Astronomical Society, 1980
- The nature of OH 0739 – 14Monthly Notices of the Royal Astronomical Society, 1980
- Infrared observations of the OH source W33 AThe Astrophysical Journal, 1978
- An infrared study of the Ophiuchus dark cloudThe Astrophysical Journal, 1978
- Infrared observations of the galactic center. IV - The interstellar extinctionThe Astrophysical Journal, 1978
- Spectrophotometry of OH 26.5+0.6 from 2 to 40 micronsThe Astrophysical Journal, 1978
- Infrared spectrophotometry of OH 231.8 + 4.2 identified with OH 0739-14The Astrophysical Journal, 1976