Zobrazeno 1 - 10
of 10 254
pro vyhledávání: '"Bahramian, A"'
Autor:
Prabu, Steve, Tingay, Steven J, Bahramian, Arash, Miller-Jones, James C. A., Wood, Callan M., O'Sullivan, Shane P.
The Centaurus A radio galaxy, due to its proximity, presents itself as one of the few systems that allow the study of relativistic jet outflows at sub-parsec distances from the central supermassive black holes, with high signal to noise. We present t
Externí odkaz:
http://arxiv.org/abs/2412.01222
Autor:
Panurach, Teresa, Dage, Kristen C., Urquhart, Ryan, Plotkin, Richard M., Paul, Jeremiah D., Bahramian, Arash, Brumback, McKinley C., Galvin, Timothy J., Molina, Isabella, Miller-Jones, James C. A., Saikia, Payaswini
Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) intermediate mass black h
Externí odkaz:
http://arxiv.org/abs/2410.23335
Autor:
Karam, Rawan, Dage, Kristen C., Tetarenko, Bailey E., Brumback, McKinley C., Haggard, Daryl, Bahramian, Arash, Hu, Chin-Ping, Neilsen, Joey, Altamirano, Diego, Athukoralalage, Wasundara, Charles, Philip A., Clarkson, William I., Hickox, Ryan C., Kennea, Jamie
The MOOSE (Monitoring Observations of SMC X-1 Excursions) program uses the Neutron Star Interior Composition Explorer Mission (NICER) to monitor the high mass X-ray binary SMC X-1 during its superorbital period excursions. Here we perform X-ray spect
Externí odkaz:
http://arxiv.org/abs/2410.17307
Autor:
Anderson, G. E., Schroeder, G., van der Horst, A. J., Rhodes, L., Rowlinson, A., Bahramian, A., Chastain, S. I., Gompertz, B. P., Hancock, P. J., Laskar, T., Leung, J. K., Wijers, R. A. M. J.
Publikováno v:
2024 ApJL 975 L13
We present the radio afterglow of short gamma-ray burst (GRB) 230217A, which was detected less than 1 day after the gamma-ray prompt emission with the Australia Telescope Compact Array (ATCA) and the Karl G. Jansky Very Large Array (VLA). The ATCA ra
Externí odkaz:
http://arxiv.org/abs/2409.07686
Autor:
Hurley-Walker, N., McSweeney, S. J., Bahramian, A., Rea, N., Horvath, C., Buchner, S., Williams, A., Meyers, B. W., Strader, Jay, Aydi, Elias, Urquhart, Ryan, Chomiuk, Laura, Galvin, T. J., Zelati, F. Coti, Bailes, Matthew
We present a long-period radio transient (GLEAM-X J0704-37) discovered to have an optical counterpart, consistent with a cool main sequence star of spectral type M3. The radio pulsations occur at the longest period yet found, 2.9 hours, and were disc
Externí odkaz:
http://arxiv.org/abs/2408.15757
Autor:
Heinke, Craig O., Zheng, Junwen, Maccarone, Thomas J., Degenaar, Nathalie, Bahramian, Arash, Sivakoff, Gregory R.
Many X-ray binaries are transiently accreting. Having statistics on their recurrence times is helpful to address questions related to binary evolution and populations, as well as the physics of binary systems. We compile a catalog of known outbursts
Externí odkaz:
http://arxiv.org/abs/2407.18867
Cosmic rays travelling through interstellar space have their propagation directions repeatedly scattered by fluctuating interstellar magnetic fields. The nature of this scattering is a major unsolved problem in astrophysics, one that has resisted sol
Externí odkaz:
http://arxiv.org/abs/2406.18160
Autor:
O'Doherty, Tyrone N., Bahramian, Arash, Goodwin, Adelle J., Miller-Jones, James C. A., Orosz, Jerome A., Strader, Jay
Identifying sources exhibiting ellipsoidal variability in large photometric surveys is becoming a promising method to search for candidate detached black holes in binaries. This technique aims to exploit the orbital-phase dependent modulation in opti
Externí odkaz:
http://arxiv.org/abs/2405.17772
Autor:
Wood, Callan M., Miller-Jones, James C. A., Bahramian, Arash, Tingay, Steven J., Prabu, Steve, Russell, Thomas D., Atri, Pikky, Carotenuto, Francesco, Altamirano, Diego, Motta, Sara E., Hyland, Lucas, Reynolds, Cormac, Weston, Stuart, Fender, Rob, Körding, Elmar, Maitra, Dipankar, Markoff, Sera, Migliari, Simone, Russell, David M., Sarazin, Craig L., Sivakoff, Gregory R., Soria, Roberto, Tetarenko, Alexandra J., Tudose, Valeriu
Multi-wavelength polarimetry and radio observations of Swift J1727.8-1613 at the beginning of its recent 2023 outburst suggested the presence of a bright compact jet aligned in the north-south direction, which could not be confirmed without high angu
Externí odkaz:
http://arxiv.org/abs/2405.12370
Publikováno v:
Journal of Irrigation and Drainage Engineering. 148