Issue |
A&A
Volume 434, Number 1, April IV 2005
|
|
---|---|---|
Page(s) | 181 - 187 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361:20042010 | |
Published online | 01 April 2005 |
Molecular hydrogen kinematics in the ring-like planetary nebula NGC 6781
Instituto de Astronomía, UNAM Campus Ensenada, Apdo. Postal 877, Ensenada, BC 22800, México e-mail: hiriart@astrosen.unam.mx
Received:
15
September
2004
Accepted:
10
December
2004
This paper presents the radial velocity mapping of the
molecular hydrogen in the ring-like planetary nebula NGC 6781.
Observations of the H2 S(1) emission line (2.122 μm,
μm) were obtained by Fabry-Pérot
spectroscopy. These observations provide a very detailed map of the
kinematic structure of the molecular hydrogen envelope in
NGC 6781. The kinematic structure is explained with a model consisting
of a thin hollow cylinder whose axis is tilted with respect to the
line of sight, and gas expanding radially outward with a velocity
proportional to the distance to the central star. Molecular hydrogen
emission was detected at LSR velocities ranging from -6.2 to +57.1 km s-1, with peak intensities between +15.7 and +25.5 km s-1. There is evidence that the molecular hydrogen
envelope is excited by shocks from the ionization front. The mass of
molecular gas is estimated to be of the order of 0.2
. The
emergent picture from the H2 kinematic structure supports the
scenario where the structure of NGC 6781 was formed from the
ionization and destruction of an ellipsoidal molecular envelope that
began with the destruction and ionization of the least dense polar
caps and will continue until the densest molecular material at nebular
waist is fully ionized.
Key words: ISM: molecules / ISM: planetary nebulae: general / ISM: planetary nebulae: individual: NGC 6781
© ESO, 2005
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