A CNO dichotomy among O2 giant spectra in the magellanic clouds

Astrophysical Journal

Volumn 608, Issue 2 I, 2004, Pages 1028-1038

  Walborn, Nolan R ^a   Morrell, Nidia I ^b,g,h,i   Howarth, Ian D ^c   Crowther, Paul A ^d,j   Lennon, Daniel J ^e   Massey, Philip ^f,h   Arias, Julia I ^g,h,i  

^a AURA for the European Space Agency   (United States)

^b LAS CAMPANAS OBSERVATORY   (Chile)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

^d UNIVERSITY OF SHEFFIELD   (United Kingdom)

^e ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^f LOWELL OBSERVATORY   (United States)

^g UNIVERSIDAD NACIONAL DE LA PLATA   (Argentina)

^h NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

ⁱ Universidad Nacional del Litoral   (Argentina)

^j European Southern Observatory   (United Kingdom)

more..

Author keywords

Magellanic Clouds; Stars: abundances; Stars: early type; Stars: evolution; Stars: fundamental parameters

Indexed keywords

EID: 3142781548     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/420761     Document Type: Review

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