Numerical models for the 19th century outbursts of η Carinae

Details Numerical models for the 19th century outbursts of η Carinae Numerical models for the 19th century outbursts of η Carinae

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..190g&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

We present here 2D hydrodynamical simulations of the eruptive events of the 1840s and the 1890s eruptions suffered by the massive star η Car. We assume a colliding wind scenario to explain the shape and kinematics of the bipolar nebulae formed from these events. We also find the formation of some tenuous, equatorial, high-speed features that seem to be related to the observed equatorial skirt of η Car.

Affiliated with

Also associated with

No associations

Rating

Numerical models for the 19th century outbursts of η Carinae 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 Numerical models for the 19th century outbursts of η Carinae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical models for the 19th century outbursts of η Carinae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674248