New Star
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Observed 9/2/2026
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Observed 9/2/2026
We carried out a systematic search for new star clusters in a field of 5$^{\circ} \times5^{\circ}$ centred close to the
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Observed 9/2/2026
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Observed 9/2/2026
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Observed 8/18/2026
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Observed 8/18/2026
We find a new mechanism of neutron star radiation wherein radiation is produced by the stellar interior. The source of
We study the cooling behaviour of an isolated strange quark star, using an equation of state derived from perturbative QCD
We present a review of recent studies of the formation and evolution of the Milky Way galaxy, in particular based
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Observed 8/18/2026
We summarise recent developments on synthesis models for massive star populations with a particular emphasis on Wolf-Rayet (WR) stars. Quantitative
71 Tau was discovered to be a $δ$ Scuti star by Horan (1979, AJ 84, 1770). To our knowledge no
HadV98 = CoD-22 12017 = GSC 6825.253 is a variable star discovered by Katsumi Haseda. This object has been recently
Subdwarf B (sdB) stars are thought to be helium burning stars with low mass hydrogen envelopes. Several evolutionary paths have
We have invented a new algorithm to use with self-gravitating SPH Star Formation codes. The new method is designed to
The past decade has led to significant improvements in our understanding of the physical structure of the molecular cores of
Star-forming regions have been the targets of X-ray observations since the dawn of satellite X-ray astronomy. The increase in sensitivity
Photometric and spectroscopic observations and analysis of the eccentric eclipsing binary V459 Cassiopeiae (e=0.0244) were performed by Lacy et al.
In the framework of the model motivated by perturbative calculations in the fourth $O(α^3_sα)$-order, the estimates for the $γp$ cross-section
The Galactic Anticenter Stellar Structure (GASS) has been identified with excess surface densities of field stars in several large area
We explore, using an exact cooling code, the thermal evolution of a neutron star undergoing episodes of intense accretion, alternated
We are conducting a large survey of star formation within ~400 nearby spiral and irregular galaxies through imaging of the