Long term optical variability of two HMXB
R Nesci, M Fiocchi, A Vagnozzi - arXiv preprint arXiv:2403.15746, 2024 - arxiv.org
We discuss the optical light curves of two Be X-ray Binaries, IGR J06074+ 2205 and SAX
J2103. 5+ 4545 recovered from the ATLAS, ZTF and ASAS-SN databases. Both sources …
J2103. 5+ 4545 recovered from the ATLAS, ZTF and ASAS-SN databases. Both sources …
Seçilen Nötron Yıldızı Bileşenli X-ışın Çiftlerinin Korunumsuz Evrim Modelleri
Bu çalışmada, geri-tür bir optik bileşen ve bir nötron yıldız barındıran düşük kütleli bazı X-ışın
çiftlerinin (NS-LMXB) korunumsuz evrim modelleri MESA evrim kodu kullanılarak elde …
çiftlerinin (NS-LMXB) korunumsuz evrim modelleri MESA evrim kodu kullanılarak elde …
[图书][B] Long-Term Visible Light Curves of Low-Mass X-Ray Binaries and Old Novae, from the Catalina Real-Time Transient Survey
CL Spencer - 2022 - search.proquest.com
As some stars progress down their evolutionary path in a close binary system, a few of the
primary stars successfully evolve via mass transfer into a white dwarf, neutron star, or black …
primary stars successfully evolve via mass transfer into a white dwarf, neutron star, or black …