Search Results - (Author, Cooperation:A. Finoguenov)
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1J. P. Dietrich ; N. Werner ; D. Clowe ; A. Finoguenov ; T. Kitching ; L. Miller ; A. Simionescu
Nature Publishing Group (NPG)
Published 2012Staff ViewPublication Date: 2012-07-06Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Staff View
ISSN: 1562-6873Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract New optical and X-ray observations of the supernova remnant (SNR) G78.2+2.1 are presented. CCD Hα observations with a Fabry-Perot interferometer attached to the 125-cm reflector at the Crimean Station of the Sternberg Astronomical Institute are used to obtain the radial-velocity field toward the SNR and in its vicinity. The brightness distribution and X-ray spectrum of the SNR are obtained from archival ROSAT and ASCA X-ray data. The X-ray image of G78.2+2.1 exhibits a shell structure (ΔR/R≃0.3) and is generally similar to its radio image; a comparison with the radio map at ν=1.4 GHz constructed from archival VLA data reveals the coincidence of features on scales of several arcminutes at the eastern boundary of G78.2+2.1. Weak X-ray emission (an outer shell or a halo of size ≃2°) has been identified for the first time far outside G78.2+2.1. The X-ray emission from G78.2+2.1 is shown to characterize a young adiabatic SNR [M X-ray ≃ 100 M ⊙, V s≃103km s−1, t≃(5–6)×103 years], which probably expands inside the cavity swept up by the progenitor's stellar wind. Searches for the corresponding radio structure are required to elucidate the nature of the outer X-ray shell or halo.Type of Medium: Electronic ResourceURL: -
3Staff View
Publication Date: 2018-03-06Publisher: Oxford University PressPrint ISSN: 0035-8711Electronic ISSN: 1365-2966Topics: PhysicsPublished by: