Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Krauss, Miriam"'
Autor:
Chomiuk, Laura, Linford, Justin D., Aydi, Elias, Bannister, Keith W., Krauss, Miriam I., Mioduszewski, Amy J., Mukai, Koji, Nelson, Thomas J., Rupen, Michael P., Ryder, Stuart D., Sokoloski, Jennifer L., Sokolovsky, Kirill V., Strader, Jay, Filipovic, Miroslav D., Finzell, Tom, Kawash, Adam, Kool, Erik C., Metzger, Brian D., Nyamai, Miriam M., Ribeiro, Valerio A. R. M., Roy, Nirupam, Urquhart, Ryan, Weston, Jennifer
We present radio observations (1--40 GHz) for 36 classical novae, representing data from over five decades compiled from the literature, telescope archives, and our own programs. Our targets display a striking diversity in their optical parameters (e
Externí odkaz:
http://arxiv.org/abs/2107.06251
Autor:
Villar-Gouy, Keila R., Salmon, Carlos Ernesto Garrido, Salvatori, Roberto, Kellner, Michael, Krauss, Miriam P. O., Rocha, Tâmara O., de Souza, Erick Almeida, Batista, Vanderlan O., Leal, Ângela C., Santos, Lucas B., Melo, Enaldo V., Oliveira-Santos, Alécia A., Oliveira, Carla R. P., Campos, Viviane C., Santos, Elenilde G., Santana, Nathalie O., Pereira, Francisco A., Amorim, Rivia S., Donato-Junior, José, Filho, José Augusto Soares Barreto
Publikováno v:
Journal of Endocrinological Investigation; Nov2024, Vol. 47 Issue 11, p2797-2807, 11p
Autor:
Weston, Jennifer H. S., Sokoloski, J. L., Metzger, Brian D., Zheng, Yong, Chomiuk, Laura, Krauss, Miriam I., Linford, Justin, Nelson, Thomas, Mioduszewski, Amy, Rupen, Michael P., Finzell, Tom, Mukai, Koji
The importance of shocks in nova explosions has been highlighted by Fermi's discovery of \gamma-ray producing novae. Over three years of multi-band VLA radio observations of the 2010 nova V1723 Aql show that shocks between fast and slow flows within
Externí odkaz:
http://arxiv.org/abs/1505.05879
Autor:
Krauss, Miriam Ilana
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2007.
Includes bibliographical references (p. 133-150).
In this thesis, I present work spanning a variety of topics relating to neutron star lowmass X-ray binaries (L
Includes bibliographical references (p. 133-150).
In this thesis, I present work spanning a variety of topics relating to neutron star lowmass X-ray binaries (L
Externí odkaz:
http://hdl.handle.net/1721.1/45408
Autor:
Chomiuk, Laura, Nelson, Thomas, Mukai, Koji, Sokoloski, J. L., Rupen, Michael P., Page, Kim L., Osborne, Julian P., Kuulkers, Erik, Mioduszewski, Amy J., Roy, Nirupam, Weston, Jennifer, Krauss, Miriam I.
Publikováno v:
2014, ApJ, 788, 130
The recurrent nova T Pyx underwent its sixth historical outburst in 2011, and became the subject of an intensive multi-wavelength observational campaign. We analyze data from the Swift and Suzaku satellites to produce a detailed X-ray light curve aug
Externí odkaz:
http://arxiv.org/abs/1404.3210
Autor:
Chakraborti, Sayan, Soderberg, Alicia, Chomiuk, Laura, Kamble, Atish, Yadav, Naveen, Ray, Alak, Hurley, Kevin, Margutti, Raffaella, Milisavljevic, Dan, Bietenholz, Michael, Brunthaler, Andreas, Pignata, Giuliano, Pian, Elena, Mazzali, Paolo, Fransson, Claes, Bartel, Norbert, Hamuy, Mario, Levesque, Emily, MacFadyen, Andrew, Dittmann, Jason, Krauss, Miriam, Briggs, M. S., Connaughton, V., Yamaoka, K., Takahashi, T., Ohno, M., Fukazawa, Y., Tashiro, M., Terada, Y., Murakami, T., Goldsten, J., Barthelmy, S., Gehrels, N., Cummings, J., Krimm, H., Palmer, D., Golenetskii, S., Aptekar, R., Frederiks, D., Svinkin, D., Cline, T., Mitrofanov, I. G., Golovin, D., Litvak, M. L., Sanin, A. B., Boynton, W., Fellows, C., Harshman, K., Enos, H., von Kienlin, A., Rau, A., Zhang, X., Savchenko, V.
Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly usually within days, because their low-mass ejecta rapidly sweep up a
Externí odkaz:
http://arxiv.org/abs/1402.6336
Autor:
Weston, Jennifer H. S., Sokoloski, Jennifer L., Zheng, Yong, Chomiuk, Laura, Mioduszewski, Amy, Mukai, Koji, Rupen, Michael P., Krauss, Miriam I., Roy, Nirupam, Nelson, Thomas
Publikováno v:
2014, ASP Conference Series, 490, 339
The radio light curves of novae rise and fall over the course of months to years, allowing for detailed observations of the evolution of the nova shell. However, the main parameter determined by radio models of nova explosions - the mass of the eject
Externí odkaz:
http://arxiv.org/abs/1306.2265
Autor:
Roy, Nirupam, Chomiuk, Laura, Sokoloski, Jennifer L., Weston, Jennifer, Rupen, Michael P., Johnson, Traci, Krauss, Miriam I., Nelson, Thomas, Mukai, Koji, Mioduszewski, Amy, Bode, Michael F., Eyres, Stewart P. S., O'Brien, Tim J.
Publikováno v:
2012, Bulletin of the ASI, 40, 293
Novae, which are the sudden visual brightening triggered by runaway thermonuclear burning on the surface of an accreting white dwarf, are fairly common and bright events. Despite their astronomical significance as nearby laboratories for the study of
Externí odkaz:
http://arxiv.org/abs/1302.4455
Autor:
Nelson, Thomas, Chomiuk, Laura, Roy, Nirupam, Sokoloski, J. L., Mukai, Koji, Krauss, Miriam I., Mioduszewski, Amy J., Rupen, Michael P., Weston, Jennifer
Publikováno v:
2014, ApJ, 785, 78
Despite being the prototype of its class, T Pyx is arguably the most unusual and poorly understood recurrent nova. Here, we use radio observations from the Karl G. Jansky Very Large Array to trace the evolution of the ejecta over the course of the 20
Externí odkaz:
http://arxiv.org/abs/1211.3112
Autor:
Chomiuk, Laura, Krauss, Miriam I., Rupen, Michael P., Nelson, Thomas, Roy, Nirupam, Sokoloski, Jennifer L., Mukai, Koji, Munari, Ulisse, Mioduszewski, Amy, Weston, Jennifer, O'Brien, Tim J., Eyres, Stewart P. S., Bode, Michael F.
Publikováno v:
2012, ApJ, 761, 173
We present multi-frequency radio observations of the 2010 nova event in the symbiotic binary V407 Cygni, obtained with the Karl G. Jansky Very Large Array and spanning 1-45 GHz and 17-770 days following discovery. This nova---the first ever detected
Externí odkaz:
http://arxiv.org/abs/1210.6029