A kinematical study of the jet GGD 34

Details A kinematical study of the jet GGD 34 A kinematical study of the jet GGD 34

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...267..559g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 267, no. 2, p. 559-565.

Astronomy and Astrophysics

Astronomy

8

Plasma Jets, Radial Velocity, Stellar Mass Ejection, Stellar Physics, Astronomical Spectroscopy, Infrared Astronomy, Space Observations (From Earth), Velocity Distribution

Scientific paper

Results are presented of an analysis of CCD images and high-resolution spectra of GGD 34 object, obtained in July 1988 (imaging) and August 1989 (long-slit spectroscopy) with the 3.5 m telescope of the Calar Alto Observatory (Almeria, Spain). GGD 34, which is in a well known region of star formation NGC 7129, is a jet consisting of three major condensations separated 0.08 pc from each other and aligned over 0.17 pc in the east-west direction. As a result of the present analyses, the main physical parameters of GGD 34 are obtained and the constraints imposed by the velocity field of the flow to the hydrodynamics of the jet are determined. The characteristics of GGD 34 suggest that it is a jet undergoing a 'kink' instability.

Affiliated with

Also associated with

No associations

Rating

A kinematical study of the jet GGD 34 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A kinematical study of the jet GGD 34, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A kinematical study of the jet GGD 34 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1771597