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Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1.
Krawczynski H, Muleri F, Dovčiak M, Veledina A, Rodriguez Cavero N, Svoboda J, Ingram A, Matt G, Garcia JA, Loktev V, Negro M, Poutanen J, Kitaguchi T, Podgorný J, Rankin J, Zhang W, Berdyugin A, Berdyugina SV, Bianchi S, Blinov D, Capitanio F, Di Lalla N, Draghis P, Fabiani S, Kagitani M, Kravtsov V, Kiehlmann S, Latronico L, Lutovinov AA, Mandarakas N, Marin F, Marinucci A, Miller JM, Mizuno T, Molkov SV, Omodei N, Petrucci PO, Ratheesh A, Sakanoi T, Semena AN, Skalidis R, Soffitta P, Tennant AF, Thalhammer P, Tombesi F, Weisskopf MC, Wilms J, Zhang S, Agudo I, Antonelli LA, Bachetti M, Baldini L, Baumgartner WH, Bellazzini R, Bongiorno SD, Bonino R, Brez A, Bucciantini N, Castellano S, Cavazzuti E, Ciprini S, Costa E, De Rosa A, Del Monte E, Di Gesu L, Di Marco A, Donnarumma I, Doroshenko V, Ehlert SR, Enoto T, Evangelista Y, Ferrazzoli R, Gunji S, Hayashida K, Heyl J, Iwakiri W, Jorstad SG, Karas V, Kolodziejczak JJ, La Monaca F, Liodakis I, Maldera S, Manfreda A, Marscher AP, Marshall HL, Mitsuishi I, Ng CY, O'Dell SL, Oppedisano C, Papitto A, Pavlov GG, Peirson AL, Perri M, Pesce-Rollins M, Pilia M, Possenti A, Puccetti S, Ramsey BD, Romani RW, Sgrò C, Slane P, Spandr… See abstract for full author list ➔ Krawczynski H, et al. Among authors: wilms j. Science. 2022 Nov 11;378(6620):650-654. doi: 10.1126/science.add5399. Epub 2022 Nov 3. Science. 2022. PMID: 36356134
Cygnus X-1 contains a 21-solar mass black hole-Implications for massive star winds.
Miller-Jones JCA, Bahramian A, Orosz JA, Mandel I, Gou L, Maccarone TJ, Neijssel CJ, Zhao X, Ziółkowski J, Reid MJ, Uttley P, Zheng X, Byun DY, Dodson R, Grinberg V, Jung T, Kim JS, Marcote B, Markoff S, Rioja MJ, Rushton AP, Russell DM, Sivakoff GR, Tetarenko AJ, Tudose V, Wilms J. Miller-Jones JCA, et al. Among authors: wilms j. Science. 2021 Mar 5;371(6533):1046-1049. doi: 10.1126/science.abb3363. Epub 2021 Feb 18. Science. 2021. PMID: 33602863
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: wilms j. Science. 2017 Feb 24;355(6327):817-819. doi: 10.1126/science.aai8635. Epub 2017 Feb 20. Science. 2017. PMID: 28219970 Free article.