Published April 1978 | Version v1
Journal article

Is gas in the Orion nebula depleted

  • 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