Large Supernova Remnants Research Articles

Large supernova remnants as common features of the disk

The distribution of the column density of HI over the sky shows strongly organized features of large angular extent. In particular, there is (1) a conspicuous set of arching concentric filaments extending more than 80° on either side of ℓ = 330°, and (2) a prominent extended region of low column density above ℓ ∼ +40° and centered on ℓ ∼ 130°. The changes is column density in the b-direction in this region of low NH is almost step-like at ℓ ∼ +40°.

A new large supernova remnant in the southern sky?

A faint filamentary structure on a Southern Schmidt plate is thought to be a supernova remnant.

The interaction between the blast wave of a supernova remnant and interstellar clouds

view Abstract Citations (412) References (43) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The interaction between the blast wave of a supernova remnant and interstellar clouds. McKee, C. F. ; Cowie, L. L. Abstract When an interstellar (or circumstellar) cloud is overtaken by a blast wave, a shock is driven into the cloud. The velocity of the shock is derived as a function of the cloud density, and the effects of thermal conduction between the blast wave and the shocked cloud are discussed. It is shown that many of the observed features of the quasi-stationary flocculi in Cas A can be accounted for by this model. Some aspects of the evolution of supernova remnants (SNRs) in a cloudy interstellar medium are discussed. It is argued that the optically observed filaments in older SNRs represent shocked interstellar clouds with a significantly lower velocity than the blast wave propagating in the intercloud medium. The dynamics of large SNRs are relatively unaffected by interstellar clouds. It is suggested that most optically observed SNRs are still in the adiabatic phase of their expansion. Application of results to the Cygnus Loop shows that Woltjer's interpretation of the optical and X-ray observations is self-consistent. Vela X and Shajn 147 are also briefly discussed. Publication: The Astrophysical Journal Pub Date: February 1975 DOI: 10.1086/153373 Bibcode: 1975ApJ...195..715M Keywords: Interstellar Gas; Shock Heating; Shock Wave Interaction; Supernova Remnants; Abundance; Astronomical Models; Cloud Physics; Light Emission; Stellar Evolution; X Ray Astronomy; Astrophysics full text sources ADS | data products SIMBAD (1)