[WC] Stellar Wind Turbulent Outflows Feeding the ISM

Details [WC] Stellar Wind Turbulent Outflows Feeding the ISM [WC] Stellar Wind Turbulent Outflows Feeding the ISM

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12...90g&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

1

Instabilities, Line: Profiles, Planetary Nebulae, Stars: Wolf-Rayet, Stars: Mass-Loss

Scientific paper

Wind fluctuations in [WC 8-9]-type central stars of planetary nebulae have been detected. Moving features seen on the top of the C III lambda 5696 and C IV lambda lambda 5801/12 emission lines of HD 826 (NGC 40) and BD +30^o3639 are interpreted as outflowing clumps which are radially accelerated in the Wolf-Rayet winds. Kinematic parameters of the blobs were derived and compared to those observed for massive Wolf-Rayet stars.

Affiliated with

Also associated with

No associations

Rating

[WC] Stellar Wind Turbulent Outflows Feeding the ISM 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 [WC] Stellar Wind Turbulent Outflows Feeding the ISM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and [WC] Stellar Wind Turbulent Outflows Feeding the ISM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1043215