Results 91 to 100 of about 403,855 (253)
NICER, NuSTAR, and Insight-HXMT Views to Black Hole X-Ray Binary SLX 1746–331
The Astrophysical Journal LettersWe study the spectral and temporal properties of the black hole (BH) X-ray transient binary SLX 1746–331 during the 2023 outburst with NICER, NuSTAR, and Insight-HXMT observations.Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui, Shuang-Nan Zhang, Yu-Peng Chen, Ling-Da Kong, Zhuo-Li Yu, Long Ji, Peng-Ju Wang, Ming-Yu Ge, Jin-Lu Qu, Lian Tao, Zhi Chang, Jian Li, Zhao-sheng Li, Zhe Yan +15 moredoaj +1 more sourceUltraluminous X-ray binaries
Ultraluminous X-ray binaries have challenged our assumptions of extreme accretion rates in X-ray binaries, and impact other subfields of astronomy, such as cosmology, gravitational wave sources and supernovæ. Our understanding of ULXs has changed tremendously over the last 35 years, and we now know that ULXs can be powered by accreting neutron stars as Dage, Kristen C., Kovlakas, Konstantinosopenaire +2 more sourcesInsight-HXMT, NICER, and NuSTAR Views to the Newly Discovered Black Hole X-Ray Binary Swift J151857.0–572147
The Astrophysical Journal LettersThe systematic properties are largely unknown for the black hole X-ray binary Swift J151857.0–572147 newly discovered in the 2024 outburst. The nature of a black hole can be completely defined by specifying the mass and dimensionless spin parameter ...Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui, Yu-Peng Chen, Shuang-Nan Zhang, Ling-Da Kong, A. Santangelo, Zhuo-Li Yu, Long Ji, Peng-Ju Wang, Zhi Chang, Jian Li, Zhao-sheng Li +12 moredoaj +1 more sourceInsight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070. [PDF]
Nat Commun, 2021 You B, Tuo Y, Li C, Wang W, Zhang SN, Zhang S, Ge M, Luo C, Liu B, Yuan W, Dai Z, Liu J, Qiao E, Jin C, Liu Z, Czerny B, Wu Q, Bu Q, Cai C, Cao X, Chang Z, Chen G, Chen L, Chen T, Chen Y, Chen Y, Chen Y, Cui W, Cui W, Deng J, Dong Y, Du Y, Fu M, Gao G, Gao H, Gao M, Gu Y, Guan J, Guo C, Han D, Huang Y, Huo J, Jia S, Jiang L, Jiang W, Jin J, Jin Y, Kong L, Li B, Li C, Li G, Li M, Li T, Li W, Li X, Li X, Li X, Li Y, Li Z, Liang X, Liao J, Liu C, Liu G, Liu H, Liu X, Liu Y, Lu B, Lu F, Lu X, Luo Q, Luo T, Ma X, Meng B, Nang Y, Nie J, Ou G, Qu J, Sai N, Shang R, Song L, Song X, Sun L, Tan Y, Tao L, Wang C, Wang G, Wang J, Wang L, Wang W, Wang Y, Wen X, Wu B, Wu B, Wu M, Xiao G, Xiao S, Xiong S, Xu Y, Xu Y, Yang J, Yang S, Yang Y, Yi Q, Yin Q, You Y, Zhang A, Zhang C, Zhang F, Zhang H, Zhang J, Zhang T, Zhang W, Zhang W, Zhang W, Zhang Y, Zhang Y, Zhang Y, Zhang Y, Zhang Z, Zhang Z, Zhao H, Zhao X, Zheng S, Zhou D, Zhou J, Zhu Y, Zhu Y. +126 moreeuropepmc +1 more sourceMulti-wavelength properties of IGR J05007-7047 (LXP 38.55) and
identification as a Be X-ray binary pulsar in the LMC
, 2016 We report on the results of a $\sim$40 d multi-wavelength monitoring of the
Be X-ray binary system IGR J05007-7047 (LXP 38.55). During that period the
system was monitored in the X-rays using the Swift telescope and in the optical
with multiple ...Delvaux, C., Haberl, F., Sturm, R., Udalski, A., Vasilopoulos, G. +4 morecore +1 more sourceAn Optical Search for New Outbursting Low Mass X-Ray Binaries
The Astrophysical JournalTransient low-mass X-ray binaries (LMXBs) are discovered largely by X-ray and gamma-ray all-sky monitors. The X-ray outburst is also accompanied by an optical brightening, which empirically can precede the detection of X-rays.Yuankun Wang, Eric C. Bellm, Allison Crossland, William I. Clarkson, Alessandro Mazzi, Reed Riddle, Russ R. Laher, Ben Rusholme +7 moredoaj +1 more sourceA ROSAT Survey of Contact Binary Stars
, 2005 Contact binary stars are common variable stars which are all believed to emit
relatively large fluxes of x-rays. In this work we combine a large new sample
of contact binary stars derived from the ROTSE-I telescope with x-ray data from
the ROSAT All-Sky ...Hunsch M., M. T. Geske, McGale P. A., S. J. Gettel, T. A. McKay, Voges W. +5 morecore +1 more sourceX-Ray Polarized View of the Accretion Geometry in the X-Ray Binary Circinus X-1
The Astrophysical Journal LettersCir X-1 is a neutron star X-ray binary characterized by strong variations in flux during its eccentric ∼16.6 day orbit. There are also strong variations in the spectral state, and it has historically shown both atoll and Z state properties.John Rankin, Fabio La Monaca, Alessandro Di Marco, Juri Poutanen, Anna Bobrikova, Vadim Kravtsov, Fabio Muleri, Maura Pilia, Alexandra Veledina, Rob Fender, Philip Kaaret, Dawoon E. Kim, Andrea Marinucci, Herman L. Marshall, Alessandro Papitto, Allyn F. Tennant, Sergey S. Tsygankov, Martin C. Weisskopf, Kinwah Wu, Silvia Zane, Filippo Ambrosino, Ruben Farinelli, Andrea Gnarini, Iván Agudo, Lucio A. Antonelli, Matteo Bachetti, Luca Baldini, Wayne H. Baumgartner, Ronaldo Bellazzini, Stefano Bianchi, Stephen D. Bongiorno, Raffaella Bonino, Alessandro Brez, Niccolò Bucciantini, Fiamma Capitanio, Simone Castellano, Elisabetta Cavazzuti, Chien-Ting Chen, Stefano Ciprini, Enrico Costa, Alessandra De Rosa, Ettore Del Monte, Laura Di Gesu, Niccolò Di Lalla, Immacolata Donnarumma, Victor Doroshenko, Michal Dovčiak, Steven R. Ehlert, Teruaki Enoto, Yuri Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier A. Garcia, Shuichi Gunji, Kiyoshi Hayashida, Jeremy Heyl, Wataru Iwakiri, Svetlana G. Jorstad, Vladimir Karas, Fabian Kislat, Takao Kitaguchi, Jeffery J. Kolodziejczak, Henric Krawczynski, Luca Latronico, Ioannis Liodakis, Simone Maldera, Alberto Manfreda, Frédéric Marin, Alan P. Marscher, Francesco Massaro, Giorgio Matt, Ikuyuki Mitsuishi, Tsunefumi Mizuno, Michela Negro, Chi-Yung Ng, Stephen L. O’Dell, Nicola Omodei, Chiara Oppedisano, George G. Pavlov, Abel L. Peirson, Matteo Perri, Melissa Pesce-Rollins, Pierre-Olivier Petrucci, Andrea Possenti, Simonetta Puccetti, Brian D. Ramsey, Ajay Ratheesh, Oliver J. Roberts, Roger W. Romani, Carmelo Sgrò, Patrick Slane, Paolo Soffitta, Gloria Spandre, Douglas A. Swartz, Toru Tamagawa, Fabrizio Tavecchio, Roberto Taverna, Yuzuru Tawara, Nicholas E. Thomas, Francesco Tombesi, Alessio Trois, Roberto Turolla, Jacco Vink, Fei Xie +103 moredoaj +1 more source