Volume 377, Number 3, October III 2001
|Page(s)||1042 - 1055|
|Published online||15 October 2001|
Instituto Nacional de Astrofísica, Óptica y Electrónica INAOE, Apdo Postal 51 y 216, 72000 Puebla, Pue., México
2 Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Santa Cruz de La Palma, Canarias, Spain e-mail: firstname.lastname@example.org
3 Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Canarias, Spain e-mail: email@example.com
Corresponding author: M. Rodríguez, firstname.lastname@example.org
Accepted: 6 August 2001
We present low and high resolution long-slit spectra of three bipolar planetary nebulae (PNe) with bright central cores: A 79, He 2-428 and M 1-91. He 2-428 and M 1-91 have high density (from 103.3 to 106.5 cm-3) unresolved nebular cores that indicate that strong mass loss/exchange phenomena are occurring close to their central stars. An F0 star is found at the centre of symmetry of A 79; its reddening and distance are consistent with the association of the star with the nebula. The spectrum of the core of He 2-428 shows indications of the presence of a hot star with red excess emission, probably arising in a late-type companion. A 79 is one of the richest PNe in and , the abundances of M 1-91 are at the lower end of the range spanned by bipolar PNe, and He 2-428 shows very low abundances, similar to those measured for halo PNe. The extended nebulae of A 79 and He 2-428 have inclined equatorial rings expanding at a velocity of ~15 km s-1, with kinematical ages ≥104 yrs. The association of these aged, extended nebulae with a dense nebular core (He 2-428) or a relatively late type star (A 79) is interpreted as evidence for the binarity of their nuclei.
Key words: ISM: abundances / ISM: kinematics and dynamics / planetary nebulae: individual: A 79 / planetary nebulae: individual: He 2-428 / planetary nebulae: individual: M 1-91
© ESO, 2001
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