Studying the spatially resolved Schmidt-Kennicutt law in interacting galaxies: The case of Arp 158

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Boquien, M ^a,b   Lisenfeld, U ^c   Duc, P A ^d   Braine, J ^e   Bournaud, F ^d   Brinks, E ^f   Charmandaris, V ^g,h,i  

^a UNIVERSITY OF MASSACHUSETTS   (United States)

^b AIX MARSEILLE UNIVERSITÉ   (France)

^c UNIVERSITY OF GRANADA   (Spain)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

^f UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^g UNIVERSITY OF CRETE   (Greece)

^h INSTITUTE OF ELECTRONIC STRUCTURE AND LASER   (Greece)

ⁱ OBSERVATOIRE DE PARIS   (France)

Author keywords

galaxies: interactions; galaxies: star formation

Indexed keywords

COLUMN DENSITY; GALAXIES: INTERACTIONS; GALAXIES: STAR FORMATION; GRAVITATIONAL INSTABILITY; INTERACTING SYSTEM; INTERSTELLAR MEDIUMS; METALLICITIES; MOLECULAR GAS; OPTICAL SPECTROSCOPY; REGIONS OF INTEREST; SPATIALLY RESOLVED; SPECTRAL ENERGY DISTRIBUTION; SPIRAL GALAXIES; STAR FORMATION RATES; STAR FORMATIONS; STAR-FORMING REGION; STARBURSTS; STELLAR CONTENT; STELLAR POPULATIONS; SYNTHESIS CODE; YOUNG STARS;

ATOMIC SPECTROSCOPY; DEBRIS; DENSITY OF GASES; INTERNET PROTOCOLS; MERGERS AND ACQUISITIONS; SOLAR SYSTEM;

STARS;

EID: 84857170784     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117004     Document Type: Article

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