SIMBAD references

2014AJ....148...57G - Astron. J., 148, 57 (2014/September-0)

A spectroscopic and photometric study of the planetary nebulae Kn 61 and Pa 5.

GARCIA-DIAZ MA.T., GONZALEZ-BUITRAGO D., LOPEZ J.A., ZHARIKOV S., TOVMASSIAN G., BORISOV N. and VALYAVIN G.

Abstract (from CDS):

We present the first morpho-kinematical analysis of the planetary nebulae Kn 61 and Pa 5 and explore the nature of their central stars. Our analysis is based on high-resolution and medium-resolution spectroscopic observations, deep narrow-band imaging, and integral photometry. This material allows us to identify the morphological components and study their kinematics. The direct images and spectra indicate an absence of the characteristic [N II] and [S II] emission lines in both nebulae. The nebular spectrum of Kn 61 suggests a hydrogen deficient planetary nebula and the stellar spectrum of the central star reveals a hydrogen-deficient PG 1159-type star. The [O III] position velocity diagram reveals that Kn 61 is a closed, empty, spherical shell with a thin border and a filamentary surface expanding at 67.6 km/s and the shell is currently not expanding isotropically. We derived a kinematic age of ∼1.6x104 yr for an assumed distance of 4 kpc. A photometric period of ∼5.7(±0.4) days has been detected for Kn 61, indicating the presence of a possible binary system at its core. A possible link between filamentary spherical shells and PG 1159-type stars is noted. The morphology of Pa 5 is dominated by an equatorial toroid and faint polar extensions. The equatorial region of this planetary nebula is expanding at 45.2 km/s. The stellar spectrum corresponds to a very hot star and is dominated by a steep blue rising continuum and He II, Balmer, and Ca II photospheric lines.

Abstract Copyright:

Journal keyword(s): ISM: kinematics and dynamics - planetary nebulae: individual: (Kn 61, Pa 5) - techniques: imaging spectroscopy - techniques: photometric

Simbad objects: 8

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2020.02.18-08:17:58

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