The Kinematics of the S-shaped Nebula N 119 in the LMC

Details The Kinematics of the S-shaped Nebula N 119 in the LMC The Kinematics of the S-shaped Nebula N 119 in the LMC

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..167r&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Other

Galaxies: Magellanic Clouds, Stars: Wolf-Rayet, Ism: Kinematics And Dynamics, Ism: Bubbles, Ism: Individual (N 119)

Scientific paper

We present the kinematics of the nebula N 119 in the Large Magellanic Cloud. The detailed 3D spectroscopy has been carried out in the lines of Hα and [OIII] (λ5007 Å) using a scanning Fabry-Perot interferometer. Several massive stars, including a WR star, are found near the center of this nebula. We identify for the first time a Wolf-Rayet nebula formed by a WN3 star, and a wind-blown bubble formed by an O7III(f) star. Those bubbles, together with another expanding bubble (DEML 132a), contribute to give to N 119 its peculiar spiral shape. It is suggested that the strong winds of the very massive stars have excavated the original molecular cloud where the stars of the central OB association LH41 formed.

Affiliated with

Also associated with

No associations

Rating

The Kinematics of the S-shaped Nebula N 119 in the LMC 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 The Kinematics of the S-shaped Nebula N 119 in the LMC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Kinematics of the S-shaped Nebula N 119 in the LMC will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1807745