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搜索结果: 1-15 共查到天文学 Supernova Remnants相关记录25条 . 查询时间(0.046 秒)
We report the results of spectroscopic mapping observations carried out toward small (1' × 1') regions within the supernova remnants W44, W28, IC 443, and 3C 391 using the Infrared Spectrograph (IRS) ...
We present Wide Field Camera 3 images taken with the Hubble Space Telescope within a single field in the southern grand design star-forming galaxy M83. Based on their size, morphology, and photometry ...
We present the results of a study of observational and identification techniques used for surveys and spectroscopy of candidate supernova remnants (SNRs) in the Sculptor Group galaxy NGC 300. The goal...
Supernova remnants (SNRs) were often discovered in radio surveys of the Galactic plane. Because of the surface-brightness limit of previous surveys, more faint or confused SNRs await discovery. The Si...
Supernova remnants (SNRs) are a complex class of sources, and their heterogeneous nature has hindered the characterization of their general observational properties. To overcome this challenge,in thi...
We have studied the shock-excited molecular regions associated with four supernova remnants (SNRs) — IC443C, W28, W44 and 3C391 — and two Herbig-Haro objects,HH7 and HH54, using Spitzer s Infrared Sp...
The Fermi $\gamma$-ray space telescope reported the observation of several Galactic supernova remnants recently, with the $\gamma$-ray spectra well described by hadronic $pp$ collisions. The possible ...
We present the results of new Australia Telescope Compact Array (ATCA) observations of one of the largest supernova remnants, SNR J0450{709, in the Local Group of galaxies. We found that this Large Ma...
On the magnetic field evolution in shell-like supernova remnants
The composite form of the supernova remnant 3C 400.2:two interacting supernova remnants or a single supernova remnant with a blow-out?
HST Observations of Young, Oxygen-Rich Supernova Remnants
X-ray Observations of Supernova Remnants
Supernova Remnants and Molecular Clouds。
The complex relations between Supernova Remnants and Neutron Stars
Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants

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