Are young radio sources in equipartition?

Astronomy and Astrophysics

Volumn 487, Issue 3, 2008, Pages 885-894

  Orienti, M ^a,b,c   Dallacasa, D ^b,c  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSITY OF BOLOGNA   (Italy)

^c INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

Author keywords

Galaxies: active; Magnetic fields; Radiation mechanisms: non thermal; Radio continuum: general

Indexed keywords

ABSORPTION; ABSORPTION SPECTROSCOPY; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; MODELS; POPULATION STATISTICS; RADIO ASTRONOMY; RADIO WAVES;

ELECTRON POPULATIONS; EQUIPARTITION; GALAXIES: ACTIVE; HIGH FREQUENCIES; HIGH MAGNETIC FIELDS; HOT SPOTTING; LOW FREQUENCIES; MINIMUM ENERGY; MULTI-FREQUENCY; PHYSICAL CONDITIONS; RADIATION MECHANISMS: NON-THERMAL; RADIO CONTINUUM: GENERAL; RADIO SOURCES; RADIO SPECTRUMS; SPECTRAL PEAKS; SPECTRAL SHAPING; SURFACE BRIGHTNESSES; THERMAL PLASMA;

EMISSION SPECTROSCOPY;

EID: 49749146733     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809948     Document Type: Article

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