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Abstract:

This review consists essentially of three parts where we consider: (1) the structure and spectrum of the hydrogen molecule; (2) the processes that in interstellar space can lead to the forma-tion and to the dissociation of the hydrogen molecule, with the aim of establishing its abundance, both on the average and in particular regions of the Galaxy; (3) the lines originating from interstellar molecular hydrogen that could be observed from the Earth. In this last Section the possible obser-vations are classified from the point of view of the height in the atmosphere from which they have to be made. © 1966 D. Reidel Publishing Company.

Registro:

Documento: Artículo
Título:The detectability of molecular hydrogen in interstellar space
Autor:Varsavsky, C.M.
Filiación:Facultad de Ciencias Exactas y Naturales University of Buenos Aires, and Institute Argentina de Radioastronomla, Buenos Aires, Argentina
Año:1966
Volumen:5
Número:3
Página de inicio:419
Página de fin:434
DOI: http://dx.doi.org/10.1007/BF02653251
Título revista:Space Science Reviews
Título revista abreviado:Space Sci Rev
ISSN:00386308
CODEN:SPSRA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v5_n3_p419_Varsavsky

Citas:

---------- APA ----------
(1966) . The detectability of molecular hydrogen in interstellar space. Space Science Reviews, 5(3), 419-434.
http://dx.doi.org/10.1007/BF02653251
---------- CHICAGO ----------
Varsavsky, C.M. "The detectability of molecular hydrogen in interstellar space" . Space Science Reviews 5, no. 3 (1966) : 419-434.
http://dx.doi.org/10.1007/BF02653251
---------- MLA ----------
Varsavsky, C.M. "The detectability of molecular hydrogen in interstellar space" . Space Science Reviews, vol. 5, no. 3, 1966, pp. 419-434.
http://dx.doi.org/10.1007/BF02653251
---------- VANCOUVER ----------
Varsavsky, C.M. The detectability of molecular hydrogen in interstellar space. Space Sci Rev. 1966;5(3):419-434.
http://dx.doi.org/10.1007/BF02653251