Chandra/HETG and NuSTAR Observations of V750 Ara; a γ Cas-type Star钱德拉/HETG和核星观测V750 Ara：一颗γ Cas型恒星The Astrophysical JournalIF02025-11-060OAAI
Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donorASTRONOMY & ASTROPHYSICSIF5.82024-10-221OA
Revealing the state transition of Cen X-3 at high spectral resolution with ChandraASTRONOMY & ASTROPHYSICSIF5.82024-10-220OA
Chandra HETG X-Ray Spectra and Variability of π Aqr, a γ Cas-type Be StarASTROPHYSICAL JOURNAL LETTERSIF11.72024-05-012OA
Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolutionASTRONOMY & ASTROPHYSICSIF5.82022-11-1112OA
The first X-ray spectrum of the high-mass X-ray binary XTE J1855-026 during the compact object eclipseMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82022-02-100OA
X-ray variability of the HMXB Cen X-3: evidence for inhomogeneous accretion flowsMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82020-12-267OAAI
High-resolution X-ray spectroscopy of supergiant HMXB 4U 1700-37 during the compact object eclipseMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82020-12-267OA
High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flareASTRONOMY & ASTROPHYSICSIF5.82020-09-2413OA
Three discoveries of γ Cas analogues from dedicated XMM-Newton observations of Be starsMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82020-02-1819OAAI
The giant outburst of 4U 0115+634 in 2011 with Suzaku and RXTE: Minimizing cyclotron line biasesASTRONOMY & ASTROPHYSICSIF5.82020-02-136OAAI
On the Apparent Absence of Wolf-Rayet plus Neutron Star Systems: The Curious Case of WR124ASTROPHYSICAL JOURNAL LETTERSIF11.72018-12-0612OAAI
NuSTAR rules out a cyclotron line in the accreting magnetar candidate 4U2206+54MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82018-06-2011OAAI
IGR J19294+1816: a new Be-X-ray binary revealed through infrared spectroscopyMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82018-02-0911OAAI
Evidence of Compton cooling during an X-ray flare supports a neutron star nature of the compact object in 4U1700-37MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82017-10-095OAAI
A precessing Be disc as a possible model for occultation events in GX 304-1MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82017-07-047OAAI
Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray BinariesSPACE SCIENCE REVIEWSIF7.42017-03-0797PREAI
A propelling neutron star in the enigmatic Be-star γ CassiopeiaMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82016-10-2838OAAI
Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binariesASTRONOMY & ASTROPHYSICSIF5.82016-06-0642OAAI
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