Simulated X-ray emission from a single-explosion model for a supernova remnant 3C 400.2

dc.contributorSchneiter, E.M., Instituto de Ciencias Nucleares, Ciudad Universitaria, Apartado Postal 70-543, CP 04510, M�xico D.F, Mexico; De La Fuente, E., Departamento de F�sica, CUCEI, Universidad de Guadalajam, Av. Revolution, 1500 S/R Guadalajam, Jalisco, Mexico; Vel�zquez, P.F., Instituto de Ciencias Nucleares, Ciudad Universitaria, Apartado Postal 70-543, CP 04510, M�xico D.F, Mexico
dc.creatorSchneiter, E.M.
dc.creatorDe La Fuente, E.
dc.creatorVelazquez, P.F.
dc.date.accessioned2015-09-15T18:56:35Z
dc.date.accessioned2023-07-04T04:28:58Z
dc.date.available2015-09-15T18:56:35Z
dc.date.available2023-07-04T04:28:58Z
dc.date.created2015-09-15T18:56:35Z
dc.date.issued2006
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-33747519980&partnerID=40&md5=9f17bdaf08b099872c0b3cb84d9fdf3d
dc.identifierhttp://hdl.handle.net/20.500.12104/44544
dc.identifier10.1111/j.1365-2966.2006.10652.x
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7269857
dc.description.abstractWe present a single-explosion model study of the 3C 400.2 supernova remnant (SNR), made with two-dimensional axisymmetric simulations. The numerical simulations were made with the adaptive grid code YGUAZ�-A. Several initial scenarios have been tested in order to reproduce the centrally peaked X-ray emission observed for this remnant. This study reveals that the explosion of the SN inside a pre-existing stellar wind bubble successfully generates the observed morphology, when thermal conduction is included in the model. The best morphological fit is obtained at an evolution time of 21000 yr, when the total luminosity is 1.2 � 1034 erg s-1. � 2006 RAS.
dc.relationScopus
dc.relationWOS
dc.relationMonthly Notices of the Royal Astronomical Society
dc.relation371
dc.relation1
dc.relation369
dc.relation374
dc.titleSimulated X-ray emission from a single-explosion model for a supernova remnant 3C 400.2
dc.typeArticle


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