The composite form of the supernova remnant 3C 400.2: Two interacting supernova remnants or a single supernova remnant with a blow-out?

dc.contributorAmbrocio-Cruz, P., Instituto de Astronomía, Universidad Nacional Autónoma de México, México, D. F., Mexico, ITSOEH, Depto. de Ciencias Básicas, Mixquiahuala, Hgo., Mexico, UAEH Campus Tlahuelilpan, Ex-Hacienda de Tlahuelilpan s/n, Tlahuelilpan, Hgo., Mexico, ITSOEH, Depto. de Ciencias Básicas, Carretera Mixquiahuala-Tula km 2.5, 42788, Mixquiahuala, Hgo., Mexico; Rosado, M., Instituto de Astronomía, Universidad Nacional Autónoma de México, México, D. F., Mexico, Instituto de Astronomia, UNAM, Apdo. Postal 70-264, 04510 México, D. F., Mexico; De La Fuente, E., Instituto de Astronomía, Universidad Nacional Autónoma de México, México, D. F., Mexico, Instituto de Astronomía y Meteorología, Depto. de Física, Universidad de Guadalajara, Guadalajara, Jal., Mexico, Instituto de Astronomía y Meteorología, Depto. de Física, Universidad de Guadalajara, Av. Vallarta No. 2602, 44130 Guadalajara, Jalisco, Mexico
dc.creatorAmbrocio-Cruz, P.
dc.creatorRosado, M.
dc.creatorDe La Fuente, E.
dc.date.accessioned2015-11-19T18:57:50Z
dc.date.accessioned2022-11-02T14:51:16Z
dc.date.available2015-11-19T18:57:50Z
dc.date.available2022-11-02T14:51:16Z
dc.date.created2015-11-19T18:57:50Z
dc.date.issued2006
dc.identifierhttp://hdl.handle.net/20.500.12104/71264
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-34248357869&partnerID=40&md5=7c373af70ae296df655aef168e025ac7
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5005217
dc.description.abstract3C 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. Hα 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.
dc.relationRevista Mexicana de Astronomia y Astrofisica
dc.relation42
dc.relation2
dc.relation241
dc.relation249
dc.relationScopus
dc.relationWOS
dc.titleThe composite form of the supernova remnant 3C 400.2: Two interacting supernova remnants or a single supernova remnant with a blow-out?
dc.typeArticle


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