Near-infrared spectroscopy of the circumnuclear star formation regions in M100: Evidence for sequential triggering

Monthly Notices of the Royal Astronomical Society

Volumn 323, Issue 3, 2001, Pages 663-671

  Ryder, S D ^a   Knapen, J H ^b,c   Takamiya, M ^d  

^a ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^d GEMINI OBSERVATORY   (United States)

Author keywords

Galaxies: evolution; Galaxies: individual: M100; Galaxies: individual: NGC 4321; Galaxies: kinematics and dynamics; Galaxies: structure; Infrared: galaxies

Indexed keywords

GALAXIES; INFRARED DEVICES; STARS;

GALAXIES: INDIVIDUALS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY EVOLUTION; GALAXY: INDIVIDUAL: M100; GALAXY: INDIVIDUAL: NGC 4321; INFRARED GALAXIES; STAR FORMATION REGIONS; STARS FORMATION;

NEAR INFRARED SPECTROSCOPY;

EID: 0041912942     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04221.x     Document Type: Article

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