搜索结果: 1-15 共查到“理学 Supernova Remnants”相关记录26条 . 查询时间(0.075 秒)
Spitzer spectral line mapping of supernova remnants. I. Basic data and principal component analysis
Molecules Abundances
2014/12/23
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) ...
SUPERNOVA REMNANTS AND THE INTERSTELLAR MEDIUM OF M83: IMAGING AND PHOTOMETRY WITH THE WIDE FIELD CAMERA 3 ON THE HUBBLE SPACE TELESCOPE
supernova star-forming galaxy M83
2014/12/20
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 ...
A Study of Optical Observing Techniques for Extra-Galactic Supernova Remnants: Case of NGC 300
Optical Observing Techniques Extra-Galactic Supernova Remnants NGC 300
2012/2/21
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...
A Sino-German $λ$6\ cm polarization survey of the Galactic plane VI. Discovery of supernova remnants G178.2-4.2 and G25.1-2.3
supernova remnants – ISM: individual objects: G178.2− 4.2, G25.1− 2.3 – Radio continuum: ISM
2011/9/27
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...
Using the X-ray Morphologies of Young Supernova Remnants to Constrain Explosion Type, Ejecta Distribution, and Chemical Mixing
methods data analysis supernova remnants techniques image processing X-rays ISM
2010/11/10
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...
Spitzer observations of supernova remnants: II. Physical conditions and comparison with HH7 and HH54
molecular — ISM abundance — ISM clouds molecular processes shock waves
2010/11/9
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...
Neutrino emission of Fermi supernova remnants
High Energy Astrophysical Phenomena (astro-ph.HE) High Energy Physics - Phenomenology (hep-ph)
2010/12/28
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 ...
MULTIFREQUENCY OBSERVATIONS OF ONE OF THE LARGEST SUPERNOVA REMNANTS IN THE LOCAL GROUP OF GALAXIES, LMC - SNR J0450-709
ISM: supernova remnants Magellanic Clouds Radio Continuum:ISM Polarisation ISM: individual objects : SNR J0450-709
2010/10/29
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
magnetic field evolution supernova remnants
2009/7/9
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?
the supernova supernova remnant 3C 400.2
2009/6/30
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
HST Observations Supernova Remnants Oxygen-Rich
2009/6/16
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
Supernova Remnants Neutron Stars
2009/6/10
The complex relations between Supernova Remnants and Neutron Stars。
Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants
x-ray spectra Nonequilibrium ionization models supernova remnants
2009/6/5
Nonequilibrium ionization models for analysis of x-ray spectra of supernova remnants。