Direct evidence for an energetic stellar wind in NGC 6302

Details Direct evidence for an energetic stellar wind in NGC 6302 Direct evidence for an energetic stellar wind in NGC 6302

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191p...5m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, Apr. 1980, p. 5P-11P. Research supported by the Science Research C

Astronomy and Astrophysics

Astronomy

39

Astronomical Spectroscopy, Planetary Nebulae, Stellar Winds, Ionization, Line Spectra, Neon, Photon Density, Spectrum Analysis

Scientific paper

An 800 Km/s wide wing has been found on profiles of the Ne V forbidden
line at 3426 A from the wind-driven nebula NGC 6302. It is proposed that
the emission from a radiatively ionized stellar wind is being observed
for the first time.

Affiliated with

Also associated with

No associations

Rating

Direct evidence for an energetic stellar wind in NGC 6302 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 Direct evidence for an energetic stellar wind in NGC 6302, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct evidence for an energetic stellar wind in NGC 6302 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1699279