Results 81 to 90 of about 112 (94)
X-raying galaxies: a Chandra legacy. [PDF]
Proc Natl Acad Sci U S A, 2010 Wang QD.
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Fermi-LAT Observations of γ-Ray Emission toward the Outer Halo of M31. [PDF]
Astrophys J, 2019 Karwin CM +3 more
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First Results from ISO Spectra of Supernova Remnants Heavily Interacting with the ISM
Astrophysics and Space Science, 1997 ISO spectra1 of the supernova remnant RCW103 are presented. This object is the prototype of a SNR shock heavily interacting with dense ISM (probably a molecular cloud). The spectra are dominated by prominent lines and show very little continuum at » < 40 µm suggesting that the 12 and 25 µm IRAS emission from these types of remnant could be dominated by
Ernesto Oliva +4 more
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Studies of the ISM in the Vela Supernova Remnant
Astrophysics and Space Science, 2000Recent observations of the Vela SNR in the ISM species Ca II and Na I are presented and discussed in the context of the “break-down” of the Spitzer-Routly effect. Variations in line profiles with time are demonstrated, eventually through a statistical approach a description of cloud structure will be possible.
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Models for Measuring Explosion Energies and ISM Densities of Supernova Remnants in the Galaxy
, 2021 D. A. Leahy
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Inferring Properties of the ISM from Supernova Remnant Size Distributions
, 2017 Benjamin D. Elwood +2 more
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