X-ray shadows of the Draco nebula: A new method to determine total hydrogen column densities

Astronomy and Astrophysics

Volumn 336, Issue 2, 1998, Pages 682-696

  Moritz, P ^a   Wennmacher, A ^a,b   Herbstmeier, U ^a,c   Mebold, U ^a   Egger, R ^d   Snowden, S L ^d,e  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF COLOGNE   (Germany)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Dust, extinction; ISM: atoms; ISM: clouds; ISM: individual objects: Draco nebula; ISM: molecules; X rays: ISM

Indexed keywords

EID: 0038834277     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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