The influence of the cluster environment on the large-scale radio continuum emission of 8 Virgo cluster spirals

Astronomy and Astrophysics

Volumn 512, Issue 5, 2010, Pages

  Vollmer, B ^a   Soida, M ^b   Chung, A ^c   Beck, R ^d   Urbanik, M ^b   Chyzy K T ^b   Otmianowska Mazur, K ^b   Van Gorkom, J H ^e  

^a OBSERVATOIRE DE STRASBOURG   (France)

^b JAGIELLONIAN UNIVERSITY   (Poland)

^c SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

^d MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^e Columbia University ^*  (United States)

Author keywords

Galaxies: interactions; Galaxies: ISM; Galaxies: magnetic fields; Radio continuum: galaxies

Indexed keywords

MAGNETIC FIELDS; POLARIZATION;

CLUSTER ENVIRONMENTS; DEGREE OF POLARIZATION; GALACTIC DISKS; GALAXIES: INTERACTIONS; GALAXIES: ISM; RADIO CONTINUUM; RADIO CONTINUUM: GALAXIES; RADIO EMISSION; SHARP EDGES; SPIRAL GALAXIES; STAR FORMATION RATES; TOTAL POWER; WIND DIRECTIONS;

GALAXIES;

EID: 77950441861     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913591     Document Type: Article

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