Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Thomas D. Russell"'
Autor:
Thomas D. Russell, J. van den Eijnden, Payaswini Saikia, Shazrene Mohamed, Ian Heywood, G. R. Sivakoff, Rob Fender, Sara Motta, Patrick A. Woudt, James Miller-Jones
Vela X-1 is a runaway X-ray binary system hosting a massive donor star, whose strong stellar wind creates a bow shock as it interacts with the interstellar medium. This bow shock has previously been detected in H$\alpha$ and IR, but, similar to all b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c625539d0e350fcc687d00b7e0db85fe
https://ora.ox.ac.uk/objects/uuid:16ed486d-8026-4240-93ce-424c57521f4e
https://ora.ox.ac.uk/objects/uuid:16ed486d-8026-4240-93ce-424c57521f4e
Autor:
Robert Beswick, Elmar Körding, Assaf Horesh, Rob Fender, David Titterington, Sara Motta, Patrick A. Woudt, David A. H. Buckley, Stephane Corbel, David A. Green, Joe Bright, Elena Gallo, J. Moldon, Antonia Rowlinson, Ian Heywood, R. P. Armstrong, Ralph A. M. J. Wijers, Evangelia Tremou, A. J. van der Horst, Gregory R. Sivakoff, Vanessa McBride, James Miller-Jones, David R. Williams, Thomas D. Russell, Richard M. Plotkin, Alexandra J. Tetarenko, Paul J. Groot, Jeroen Homan
Publikováno v:
Nature Astron.
Nature Astron., 2020, 4 (7), pp.697-703. ⟨10.1038/s41550-020-1023-5⟩
Nature Astron., 2020, 4 (7), pp.697-+. ⟨10.1038/s41550-020-1023-5⟩
Nature Astronomy, 4, 697-703
Nature Astronomy, 697-703. Nature Publishing Group
STARTPAGE=697;ENDPAGE=703;ISSN=2397-3366;TITLE=Nature Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature Astronomy, 4, 7, pp. 697-703
Nature Astron., 2020, 4 (7), pp.697-703. ⟨10.1038/s41550-020-1023-5⟩
Nature Astron., 2020, 4 (7), pp.697-+. ⟨10.1038/s41550-020-1023-5⟩
Nature Astronomy, 4, 697-703
Nature Astronomy, 697-703. Nature Publishing Group
STARTPAGE=697;ENDPAGE=703;ISSN=2397-3366;TITLE=Nature Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature Astronomy, 4, 7, pp. 697-703
Black holes in binary systems execute patterns of outburst activity where two characteristic X-ray states are associated with different behaviours observed at radio wavelengths. The hard state is associated with radio emission indicative of a continu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64ce504df40046a24d91b7e62601cd02
https://hal.archives-ouvertes.fr/hal-02518057/document
https://hal.archives-ouvertes.fr/hal-02518057/document
Autor:
Julien Malzac, S. Drappeau, Stephane Corbel, P.-O. Petrucci, M. Péault, David M. Russell, J. L. Rodriguez, Thomas D. Russell, Mickael Coriat, Jorge Ferreira, R. Belmont, Karri I. I. Koljonen
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Monthly Notices of the Royal Astronomical Society, 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Monthly Notices of the Royal Astronomical Society, 482(2), 2447-2458. Oxford University Press
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Monthly Notices of the Royal Astronomical Society, 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 482 (2), pp.2447-2458. ⟨10.1093/mnras/sty2796⟩
Monthly Notices of the Royal Astronomical Society, 482(2), 2447-2458. Oxford University Press
The black hole candidate MAXI J1836-194 was discovered in 2011 when it went into an outburst, and was the subject of numerous, quasi-simultaneous, multi-wavelength observations in the radio, infrared, optical and X-rays. In this paper, we model its m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbfba8625a9073fad1a4f47bfd51f74d
https://hal.archives-ouvertes.fr/hal-03014168
https://hal.archives-ouvertes.fr/hal-03014168
Autor:
Carlo Ferrigno, D. de Martino, Alida Odendaal, Alessandro Papitto, Thomas D. Russell, Francesco Coti Zelati, Sergio Campana, David A. H. Buckley, S. M. Mazzola, Mariusz Gromadzki, Jian Li, Diego F. Torres, Simone Migliari, Nanda Rea, Enrico Bozzo
Publikováno v:
Astronomy & Astrophysics, 622:A211. EDP Sciences
We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim$20.1 (3300-10500 $\require{mediawiki-texvc} \AA$). The optical emissi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01b72571bcf99da37ba1f627422fce4d