Mass loss from the central star of NCG 3242

Details Mass loss from the central star of NCG 3242 Mass loss from the central star of NCG 3242

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..333h&link_type=abstract

In ESA Fourth European IUE Conf. p 333-336 (SEE N84-35135 24-88)

Computer Science

1

Data Correlation, Planetary Nebulae, Stellar Atmospheres, Stellar Mass Ejection, Stellar Winds, Atmospheric Ionization, High Resolution, Iue, Nitrogen, Stellar Composition

Scientific paper

The central star of NGC 3242 was observed with IUE in high resolution. The N V resonance doublet exhibits a weak P Cygni profile with photospheric components. Theoretical profiles are obtained from comoving-frame calculations, and the nitrogen ionization balance is computed. A mass loss rate of -10.1 to -8.1 is derived, while the final velocity is 2200 km/sec. Wind parameters compared with the parameters of the central star show that the usual relations established for winds from early-type stars are fullfilled.

Affiliated with

Also associated with

No associations

Rating

Mass loss from the central star of NCG 3242 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 Mass loss from the central star of NCG 3242, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass loss from the central star of NCG 3242 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705892