The physical structure of the point-symmetric and quadrupolar planetary nebula NGC 6309

Astronomy and Astrophysics

Volumn 481, Issue 1, 2008, Pages 107-116

  Vazquez R ^a   Miranda, L F ^b   Olguin L ^a   Ayala, S ^a,c   Torrelles, J M ^d   Contreras, M E ^a   Guillen P F ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^c CENTRO DE RADIOASTRONOMÍA Y ASTROFÍSICA   (Mexico)

^d UNIVERSITY OF BARCELONA   (Spain)

Author keywords

ISM: abundances; ISM: kinematics and dynamics; Planetary nebulae: individual: NGC 6309

Indexed keywords

CARRIER CONCENTRATION; CONTINUUM MECHANICS; DISPERSIONS; IMAGE ANALYSIS; SPECTROSCOPIC ANALYSIS;

LOW-DISPERSION SPECTROSCOPY; PLANETARY NEBULAE; RADIO CONTINUUM EMISSION;

GALAXIES;

EID: 41449086251     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078520     Document Type: Article

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