The ∑ - D relation for planetary nebulae

Astronomy and Astrophysics

Volumn 495, Issue 2, 2009, Pages 537-546

  Urosevic D ^a,e   Vukotic B ^b   Arbutina, B ^a   Ilic D ^a,e   Filipovic M ^c   Bojicic I ^d   Segan S ^a   Vidojevic S ^a  

^a UNIVERSITY OF BELGRADE   (Serbia)

^b Astronomical Observatory   (Serbia)

^c UNIVERSITY OF WESTERN SYDNEY   (Australia)

^d MACQUARIE UNIVERSITY   (Australia)

^e Isaac Newton Institute of Chile   (Serbia)

Author keywords

ISM: supernova remnants; Methods: analytical; Methods: statistical; planetary nebulae: general; Radio continuum: general; Radio continuum: ISM

Indexed keywords

GALAXIES; STARS;

ISM: SUPERNOVA REMNANTS; METHODS: ANALYTICAL; METHODS: STATISTICAL; PLANETARY NEBULAE: GENERAL; RADIO CONTINUUM: GENERAL; RADIO CONTINUUM: ISM;

PLANETARY SURFACE ANALYSIS;

EID: 61549139413     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200809494     Document Type: Article

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