The nature and structure of the emission line nebula K 3-35: A very young planetary nebula with precessing bipolar jet-like outflows?

Monthly Notices of the Royal Astronomical Society

Volumn 298, Issue 1, 1998, Pages 243-250

  Miranda, Luis F ^a   Torrelles, José M ^a,e   Guerrero, Martín A ^b   Aaquist, Orla B ^c   Eiroa, Carlos ^d  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c University Transfer Division   (Canada)

^d UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^e UNIVERSITAT DE LES ILLES BALEARS   (Spain)

Author keywords

ISM: jets and outflows; ISM: kinematics and dynamics planetary nebulae: individual: K 3 35 radio continuum: ISM; Stars: mass loss

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; GEOMETRICAL OPTICS;

EMISSION LINES; ISM JETS AND OUTFLOWS; ISM: KINEMATIC AND DYNAMIC PLANETARY NEBULA: INDIVIDUAL: K 3-35 RADIO CONTINUUM: ISM; ISM: KINEMATICS AND DYNAMICS; NARROW WIDTH; OPTICAL IMAGE; PLANETARY NEBULA; PROPERTY; RADIO CONTINUUM: ISM; STARS: MASS-LOSS;

STARS;

EID: 0039086868     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01611.x     Document Type: Article

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