The abundance gradient of NGC 1365: Evidence for a recently formed bar in an archetypal barred spiral galaxy?

Monthly Notices of the Royal Astronomical Society

Volumn 288, Issue 3, 1997, Pages 715-725

  Roy, J R ^a   Walsh, J R ^b  

^a UNIVERSITÉ LAVAL   (Canada)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxies: individual: NGC 1365; Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: spiral; H II regions; Techniques: spectroscopic

Indexed keywords

SPECTROPHOTOMETRY;

EMISSION LINES; GALAXIES: INDIVIDUAL: NGC 1365; GALAXIES: ISM; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES: NGC 1365; GALAXIES: SPIRALS; H II REGIONS; OPTICAL SPECTROPHOTOMETRY; SPIRAL GALAXIES; TECHNIQUES: SPECTROSCOPIC;

GALAXIES;

EID: 0042077503     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/288.3.715     Document Type: Article

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