The ∑ - D analysis of recently detected radio planetary nebulae in the Magellanic Clouds (Research Note)

Astronomy and Astrophysics

Volumn 503, Issue 3, 2009, Pages 855-858

  Vukotic B ^a   Urosevic D ^b,d   Filipovic M D ^c   Payne, J L ^c  

^a ASTRONOMICAL OBSERVATORY   (Serbia)

^b UNIVERSITY OF BELGRADE   (Serbia)

^c UNIVERSITY OF WESTERN SYDNEY   (Australia)

^d Isaac Newton Institute of Chile   (Serbia)

Author keywords

Galaxies Magellanic Clouds; ISM planetary nebulae general; Methods statistical; Radio continuum ISM

Indexed keywords

LARGE MAGELLANIC CLOUDS; LUMINOSITY FUNCTIONS; MAGELLANIC CLOUDS; METHODS STATISTICAL; MONTE CARLO ANALYSIS; NUMBER OF DATUM; PLANETARY NEBULAE; RADIO CONTINUUM ISM; RADIO MAPS; SURFACE BRIGHTNESS;

CLOUDS; SEA ICE; STARS;

GALAXIES;

EID: 77956990553     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911807     Document Type: Article

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