A three-position spectral line survey of sagittarius B2 between 218 and 263 GHz. II. Data analysis


Autoria(s): Nummelin, A.; Bergman, P.; Hjalmarson, A.; Friberg, P.; Irvine, W.M.; Millar, TJ; Ohishi, M.; Saito, S.
Data(s)

01/05/2000

Resumo

We present an analysis of the data from our Swedish-ESO Submillimetre Telescope molecular line survey in the 1.3 mm band of the N, M, and NW positions in the Sgr B2 molecular cloud. The line emissions from 42 molecular species, and some of their isotopomers, were analyzed assuming a single temperature and a homogeneous source. In cases where a source size much smaller than the antenna beam (23

Identificador

http://pure.qub.ac.uk/portal/en/publications/a-threeposition-spectral-line-survey-of-sagittarius-b2-between-218-and-263-ghz-ii-data-analysis(24fb204b-10fc-481f-ba6c-ffd59691fe54).html

http://www.scopus.com/inward/record.url?scp=0011070664&partnerID=8YFLogxK

Idioma(s)

eng

Direitos

info:eu-repo/semantics/restrictedAccess

Fonte

Nummelin , A , Bergman , P , Hjalmarson , A , Friberg , P , Irvine , W M , Millar , T J , Ohishi , M & Saito , S 2000 , ' A three-position spectral line survey of sagittarius B2 between 218 and 263 GHz. II. Data analysis ' Astrophysical Journal Supplement Series , vol 128 , no. 1 , pp. 213-243 .

Palavras-Chave #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science
Tipo

article