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We propose that a nonthermal X-ray arc inside the remnant of Tycho's supernova (SN) represents the interaction between the SN ejecta and the companion star's envelope lost in the impact of the explosi...
In the single degenerate (SD) scenario for Type Ia supernova (SN Ia) progenitors, an accreting white dwarf (WD) is expected to undergo a supersoft X-ray source (SSS) phase. Recently, Gilfanov & Bogdan...
Around several single DAZ and DBZ white dwarfs metal-rich disks have been observed, which are mostly believed to originate from disruption of smaller rocky planetesimals. In some cases the material do...
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the HST/ACS Coma Treasury Survey. Parameters from S\'ersic fits to the two-dimensional surface brightness distribu...
Stellar models of massive single stars are still plagued by major uncertainties. Testing and calibrating against observations is essential for their reliability.
In this paper we compute the sizes of equilateral and orthogonal shape bispectrum for the general Lorentz invariant single-field inflation. The stability of field theory implies a non-negative square ...
Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN。
The composite form of the supernova remnant 3C 400.2:two interacting supernova remnants or a single supernova remnant with a blow-out?
Non-Thermal Radio Emission from Single Hot Stars。
Is the supernova remnant 3c400.2 The result of a single supernova explosion?
The application of the basic hydrodynamical equations to globular clusters is reconsidered. As usually, these stellar systems are assumed to be spherically symmetric and in a steady state with an is...
The disk emission in the single peaked Broad Emission Lines (BELs) of Active Galactic Nuclei (AGNs) is di±cult to detect. In order to ¯nd the disk traces in BELs the line pro¯les were simu...

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