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pro vyhledávání: '"Hélène Szegedi"'
Autor:
Przemek Mróz, Krzysztof Król, Hélène Szegedi, Philip Charles, Kim L. Page, Andrzej Udalski, David A. H. Buckley, Gulab Dewangan, Pieter Meintjes, Michał K. Szymański, Igor Soszyński, Paweł Pietrukowicz, Szymon Kozłowski, Radosław Poleski, Jan Skowron, Krzysztof Ulaczyk, Mariusz Gromadzki, Krzysztof Rybicki, Patryk Iwanek, Marcin Wrona, Mateusz J. Mróz
Publikováno v:
The Astrophysical Journal Letters, Vol 977, Iss 2, p L37 (2024)
Some accreting binary systems containing a white dwarf (such as classical novae or persistent supersoft sources) are seen to emit low-energy X-rays with temperatures of ∼ 10 ^6 K and luminosities exceeding 10 ^35 erg s ^−1 . These X-rays are thou
Externí odkaz:
https://doaj.org/article/f83176292fd248369e24531bae35344d
Changes in the supercycle lengths of some SU UMa-type dwarf novae have been detected by other studies, and indicate that the mass transfer rates noticeably decrease over time. We investigated the supercycle lengths of three SU UMa-type dwarf novae: A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12f92cb0137acd657774376783078230
https://eprints.soton.ac.uk/467662/
https://eprints.soton.ac.uk/467662/