Analysis of spiral arms using anisotropic wavelets: Gas, dust and magnetic fields in M 51

Astronomy and Astrophysics

Volumn 458, Issue 2, 2006, Pages 441-452

  Patrikeev, I ^a,e   Fletcher, A ^b,c   Stepanov, R ^a   Beck, R ^b   Berkhuijsen, E M ^b   Frick, P ^a   Horellou, C ^d  

^a INSTITUTE OF CONTINUOUS MEDIA MECHANICS   (Russian Federation)

^b MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^c NEWCASTLE UNIVERSITY   (United Kingdom)

^d CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^e UNIVERSITY OF TEXAS MEDICAL BRANCH   (United States)

Author keywords

Galaxies: Individual: M 51; Galaxies: ISM; Galaxies: Magnetic fields; Galaxies: Spiral; Methods: Data analysis

Indexed keywords

ANISOTROPY; CARBON MONOXIDE; DATA REDUCTION; MAGNETIC FIELDS; WAVELET TRANSFORMS;

PITCH ANGLES; POLARIZED RADIO EMISSION; SPIRAL GALAXIES; SYSTEMATIC SHIFTS;

GALAXIES;

EID: 33750301202     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065225     Document Type: Article

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