Showing 1–20 of 40 results
/ Date/ Name
Aug 29, 2012Metallicity Effect on LMXB Formation in Globular ClustersJan 26, 2009Transient Low-Mass X-Ray Binary Populations in Elliptical Galaxies NGC 3379 and NGC 4278Mar 25, 2019Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretionJul 16, 2002Statistical properties of the energy release in emerging and evolving active regionMar 20, 2006The Eclipsing ULX in NGC 3379Apr 21, 2016The Evolution of Normal Galaxy X-ray Emission Through Cosmic History: Constraints from the 6 Ms Chandra Deep Field-SouthNov 22, 2019New insight on the far-UV SED and HeII emission from low metallicity galaxiesMar 11, 2019Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020sMar 14, 2023N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift ?Sep 9, 2008Understanding Compact Object Formation and Natal Kicks: II. The case of XTE J1118+480Feb 15, 2018The spin of the second-born black hole in coalescing binary black holesFeb 10, 2012Probing the X-Ray Binary Populations of the Ring Galaxy NGC 1291Dec 1, 2006Black Hole Formation in X-Ray Binaries: The Case of XTE J1118+480Jan 7, 2008Models for Low-Mass X-Ray Binaries in the Elliptical Galaxies NGC3379 and NGC4278: Comparison with ObservationsMar 23, 2026A quasi-star is born: formation and evolution of accreting quasi-stars as a metallicity-independent pathway to Little Red DotsFeb 27, 2019X-ray binaries as the origin of nebular HeII emission in low-metallicity star-forming galaxiesOct 25, 2017On the Spatially Resolved Star Formation History in M51 I: Hybrid UV+IR Star Formation Laws and IR Emission from Dust Heated by Old StarsJan 7, 2010Black Hole Spin-Orbit Misalignment in Galactic X-ray BinariesJun 18, 2013The Two Dimensional Projected Spatial Distribution of Globular Clusters: Method and Application to NGC4261Oct 9, 2024The effect of mass loss in models of red supergiants in the Small Magellanic Cloud