eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds
Haberl F, Maitra C, Carpano S, Dai X, Doroshenko , Dennerl K, Freyberg MJ, Sasaki M, Udalski A, Postnov KA, Shakura N (2022)
Publication Type: Journal article
Publication year: 2022
Journal
Book Volume: 661
DOI: 10.1051/0004-6361/202141878
Abstract
Context. During its performance verification phase, the soft X-ray instrument eROSITA on board the Spektrum-Roentgen-Gamma (SRG) spacecraft observed large regions in the Magellanic Clouds in which almost 40 known high-mass X-ray binaries (HMXBs, including candidates) are located.
Authors with CRIS profile
Involved external institutions
Max-Planck-Institut für extraterrestrische Physik (MPE) / Max Planck Institute for Extraterrestrial Physics
Germany (DE)
Eberhard Karls Universität Tübingen
Germany (DE)
University of Warsaw / Uniwersytet Warszawski
Poland (PL)
Lomonosov Moscow State University / Московский государственный университет имени М.В.Ломоносова
Russian Federation (RU)
Germany (DE)
Eberhard Karls Universität Tübingen
Germany (DE)
University of Warsaw / Uniwersytet Warszawski
Poland (PL)
Lomonosov Moscow State University / Московский государственный университет имени М.В.Ломоносова
Russian Federation (RU)
How to cite
APA:
Haberl, F., Maitra, C., Carpano, S., Dai, X., Doroshenko, ., Dennerl, K.,... Shakura, N. (2022). eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds. Astronomy & Astrophysics, 661. https://doi.org/10.1051/0004-6361/202141878
MLA:
Haberl, F., et al. "eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds." Astronomy & Astrophysics 661 (2022).
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