Zobrazeno 1 - 10
of 10
pro vyhledávání: '"K. I. I. Koljonen"'
The optical emission line spectra of X-ray binaries (XRBs) are thought to be produced in an irradiated atmosphere, possibly the base of a wind, located above the outer accretion disc. However, the physical nature of - and physical conditions in - the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::995a25f323232a0ba8a4659f4a420237
Autor:
I. Liodakis, K. I. I. Koljonen, D. Blinov, E. Lindfors, K. D. Alexander, T. Hovatta, M. Berton, A. Hajela, J. Jormanainen, K. Kouroumpatzakis, N. Mandarakas, K. Nilsson
Supermassive black holes have been known to disrupt passing stars producing outbursts called Tidal Disruption Events offering a unique view on the early stages of accretion disk and jet formation. The advent of large scale optical time-domain surveys
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c8033005605b197d5b8ab9747ccbc29
Autor:
G. Panizo-Espinar, M. Armas Padilla, T. Muñoz-Darias, K. I. I. Koljonen, V. A. Cúneo, J. Sánchez-Sierras, D. Mata Sánchez, J. Casares, J. Corral-Santana, R. P. Fender, F. Jiménez-Ibarra, G. Ponti, D. Steeghs, M. A. P. Torres
Publikováno v:
A&A
MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this event, the system sampled both hard and soft states following the standard evolution. We present multi-epoch optical and near-infrared spectroscopy obt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2fee4561cac5be1b847d2382def737b
https://doi.org/10.1051/0004-6361/202243426
https://doi.org/10.1051/0004-6361/202243426
Autor:
K. I. I. Koljonen, T. J. Maccarone
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 474:572-572
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f1e287b5e5511e6ec2db476af13d6877
https://doi.org/10.1093/mnras/stx2698
https://doi.org/10.1093/mnras/stx2698
Autor:
G.-B. Zhang, F. Bernardini, D. M. Russell, J. D. Gelfand, J.-P. Lasota, A. Al Qasim, A. AlMannaei, K. I. I. Koljonen, A. W. Shaw, F. Lewis, J. A. Tomsick, R. M. Plotkin, J. C. A. Miller-Jones, D. Maitra, J. Homan, P. A. Charles, P. Kobel, D. Perez, R. Doran
Publikováno v:
Astrophysical Journal; 5/1/2019, Vol. 876 Issue 1, p1-1, 1p
Publikováno v:
Astrophysical Journal; 10/1/2016, Vol. 829 Issue 2, p1-1, 1p
Autor:
F. Bernardini, D. M. Russell, A. W. Shaw, F. Lewis, P. A. Charles, K. I. I. Koljonen, J. P. Lasota, J. Casares
Publikováno v:
Astrophysical Journal Letters; 2/10/2016, Vol. 818 Issue 1, p1-1, 1p
Autor:
K. I. I. Koljonen, D. M. Russell, J. A. Fernández-Ontiveros, Sera Markoff, T. D. Russell, J. C. A. Miller-Jones, A. J. van der Horst, F. Bernardini, P. Casella, P. A. Curran, P. Gandhi, R. Soria
Publikováno v:
Astrophysical Journal; 12/1/2015, Vol. 814 Issue 2, p1-1, 1p
Autor:
Francesco Longo, Martino Marisaldi, C. Pittori, Paolo Lipari, Arnaud Ferrari, M. Prest, Sandro Mereghetti, P. W. Cattaneo, S. Sabatini, A. Pellizzoni, E. Striani, I. Lapshov, F. Perotti, S. Colafrancesco, Fulvio Gianotti, Francesco Lazzarotto, A. Giuliani, E. Rossi, Ennio Morelli, Karri I. I. Koljonen, Marco Tavani, E. Scalise, Y. Evangelista, Maura Pilia, Guy G. Pooley, M. Galli, F. Fuschino, Alessio Trois, I. Donnarumma, Massimo Rapisarda, F. Verrecchia, N. A. Nizhelskij, P. A. Caraveo, E. Del Monte, D. Zanello, L. Salotti, V. Cocco, M. Trifoglio, G. Pucella, A. Mauri, A. Rappoldi, E. Vallazza, G. De Paris, T. Contessi, G. Piano, A. W. Chen, P. Giommi, A. Argan, Andrea Bulgarelli, Enrico Costa, G. Di Persio, A. Morselli, Filippo D'Ammando, Paolo Soffitta, S. Vercellone, Michael L. McCollough, P. Picozza, P. Santolamazza, Alda Rubini, Sergei A. Trushkin, A. Zambra, M. Mastropietro, Guido Barbiellini, V. Vittorini, Marco Feroci, Luigi Pacciani, Angelo Antonelli, E. Mattaini, G. Di Cocco, Claudio Labanti
Galactic microquasars are binaries with a neutron star or stellar-mass black hole accreting gas from a companion star. They can accelerate particles to relativistic energies and emit radio flares, but the mechanism of jet energization is not known. A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd113980f3414a462dbf032ca1734b40
http://hdl.handle.net/11383/1737394
http://hdl.handle.net/11383/1737394