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Detection of large-scale X-ray bubbles in the Milky Way halo.
Predehl P, Sunyaev RA, Becker W, Brunner H, Burenin R, Bykov A, Cherepashchuk A, Chugai N, Churazov E, Doroshenko V, Eismont N, Freyberg M, Gilfanov M, Haberl F, Khabibullin I, Krivonos R, Maitra C, Medvedev P, Merloni A, Nandra K, Nazarov V, Pavlinsky M, Ponti G, Sanders JS, Sasaki M, Sazonov S, Strong AW, Wilms J. Predehl P, et al. Among authors: haberl f. Nature. 2020 Dec;588(7837):227-231. doi: 10.1038/s41586-020-2979-0. Epub 2020 Dec 9. Nature. 2020. PMID: 33299190
X-ray detection of a nova in the fireball phase.
König O, Wilms J, Arcodia R, Dauser T, Dennerl K, Doroshenko V, Haberl F, Hämmerich S, Kirsch C, Kreykenbohm I, Lorenz M, Malyali A, Merloni A, Rau A, Rauch T, Sala G, Schwope A, Suleimanov V, Weber P, Werner K. König O, et al. Among authors: haberl f. Nature. 2022 May;605(7909):248-250. doi: 10.1038/s41586-022-04635-y. Epub 2022 May 11. Nature. 2022. PMID: 35546192
A helium-burning white dwarf binary as a supersoft X-ray source.
Greiner J, Maitra C, Haberl F, Willer R, Burgess JM, Langer N, Bodensteiner J, Buckley DAH, Monageng IM, Udalski A, Ritter H, Werner K, Maggi P, Jayaraman R, Vanderspek R. Greiner J, et al. Among authors: haberl f. Nature. 2023 Mar;615(7953):605-609. doi: 10.1038/s41586-023-05714-4. Epub 2023 Mar 22. Nature. 2023. PMID: 36949334 Free PMC article.
Bright radio emission from an ultraluminous stellar-mass microquasar in M 31.
Middleton MJ, Miller-Jones JC, Markoff S, Fender R, Henze M, Hurley-Walker N, Scaife AM, Roberts TP, Walton D, Carpenter J, Macquart JP, Bower GC, Gurwell M, Pietsch W, Haberl F, Harris J, Daniel M, Miah J, Done C, Morgan JS, Dickinson H, Charles P, Burwitz V, Della Valle M, Freyberg M, Greiner J, Hernanz M, Hartmann DH, Hatzidimitriou D, Riffeser A, Sala G, Seitz S, Reig P, Rau A, Orio M, Titterington D, Grainge K. Middleton MJ, et al. Among authors: haberl f. Nature. 2013 Jan 10;493(7431):187-90. doi: 10.1038/nature11697. Epub 2012 Dec 12. Nature. 2013. PMID: 23235823
An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.
Israel GL, Belfiore A, Stella L, Esposito P, Casella P, De Luca A, Marelli M, Papitto A, Perri M, Puccetti S, Castillo GA, Salvetti D, Tiengo A, Zampieri L, D'Agostino D, Greiner J, Haberl F, Novara G, Salvaterra R, Turolla R, Watson M, Wilms J, Wolter A. Israel GL, et al. Among authors: haberl f. Science. 2017 Feb 24;355(6327):817-819. doi: 10.1126/science.aai8635. Epub 2017 Feb 20. Science. 2017. PMID: 28219970 Free article.
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