Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxaa..42..241a&link_type=abstract
Revista Mexicana de Astronomía y Astrofísica Vol. 42, pp. 241-249 (2006)
Astronomy and Astrophysics
Astronomy
1
Ism: Kinematics And Dynamics, Supernova Remnants, Supernovae: Individual (3C 400.2)
Scientific paper
3C 400.2 is a galactic supernova remnant with a complex morphology consisting of two overlapping shells of different diameters: a large shell to the southeastern side and a small shell to the northwestern side. In order to decide whether this morphology is due to two supernova explosions or to the blow-out of one supernova explosion in a medium with a density gradient, we study the kinematics of both shells. H α Fabry-Perot data are more in agreement with the scenario of only one supernova explosion undergoing a blow-out due to a density gradient in clumpy media.
Ambrocio-Cruz Patricia
de La Fuente Eduardo
Rosado Margarita
No associations
LandOfFree
The Composite Form of the Supernova Remnant 3C 400.2: Two Interacting Supernova Remnants or a Single Supernova Remnant with a Blow-Out? 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 Composite Form of the Supernova Remnant 3C 400.2: Two Interacting Supernova Remnants or a Single Supernova Remnant with a Blow-Out?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Composite Form of the Supernova Remnant 3C 400.2: Two Interacting Supernova Remnants or a Single Supernova Remnant with a Blow-Out? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1021182