Published April 1978
| Version v1
Journal article
Is gas in the Orion nebula depleted
Creators
- 1. Florence Univ. (Italy). Cattedra di Fisica dello Spazio
- 2. Osservatorio Astrofisico di Arcetri, Florence (Italy)
Description
Depletion of heavy elements has been recognized to be important in the understanding of the chemical composition of the interstellar medium. This problem is also relevant to the study of H II regions. In this paper the gaseous depletion in the physical conditions of the Orion nebula is investigated. The authors reach the conclusion that very probably no depletion of heavy elements, due to sticking on dust grains, took place during the lifetime of the Orion nebula. (Auth.)
Additional details
Publishing Information
- Journal Title
- Astrophys. Space Sci.
- Journal Volume
- 54
- Journal Issue
- 2
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 417-423
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 10419726
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ADSORPTION; CHEMICAL COMPOSITION; COSMIC DUST; COSMIC GASES; EVAPORATION; H2 REGIONS; INTERSTELLAR GRAINS; INTERSTELLAR SPACE; NEBULAE; OXYGEN
- Descriptors DEC
- COSMIC RADIO SOURCES; DUSTS; ELEMENTS; FLUIDS; GASES; NONMETALS; PARTICLES; PHASE TRANSFORMATIONS; SPACE