Other
Scientific paper
Jan 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jnanu..31..176y&link_type=abstract
J. Nanjing Univ., Vol. 31, No. 1, p. 176 - 177
Other
Emission Nebulae: Bow Shocks
Scientific paper
NGC 2359 is composed of a spherical inner shell and a fainter U-shaped outer arc seen in optical image. The WN star HD 56925 is harbored inside the filamentary shells. So far, theoretical models that have been proposed often emphasize the inner bubble, leaving the nature of the outer parabolic arc not clearly known. Here the authors propose the possibility that the outer arc of NGC 2359 is a bowshock structure other than simply a photoionization front of the clouds which happen to enclose a parabolic cavity around the WN star. The authors consider two cases in which either HD 56925 or another star is responsible for the bowshock structure.
Qu Qinyue
Wang Zhenru
Yang Chen
No associations
LandOfFree
On the wind-powered nebula NGC 2359 and the WN star HD 56925. 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 On the wind-powered nebula NGC 2359 and the WN star HD 56925., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the wind-powered nebula NGC 2359 and the WN star HD 56925. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-836170