Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy

Details Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...73h&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

H Ii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

We are performing a comprehensive spectral analysis of FUSE, IUE, HST and ground-based data of Galactic, and Large and Small Magellanic Cloud (LMC and SMC) central stars of planetary nebulae (CSPN), with the aim of understanding the overall evolution of PN in environments of differing metallicities. We determine the parameters of the central stars as well as the characteristics of the circumstellar environment.

Affiliated with

Also associated with

No associations

Rating

Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy 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 Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of Galactic and MC CSPN disclosed by Far-Ultraviolet Spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1321541