Zobrazeno 1 - 10
of 531
pro vyhledávání: '"Lyutikov, Maxim"'
Autor:
Temim, Tea, Laming, J. Martin, Kavanagh, P. J., Smith, Nathan, Slane, Patrick, Blair, William P., De Looze, Ilse, Bucciantini, Niccolò, Jerkstrand, Anders, Gountanis, Nicole Marcelina, Sankrit, Ravi, Milisavljevic, Dan, Rest, Armin, Lyutikov, Maxim, DePasquale, Joseph, Martin, Thomas, Drissen, Laurent, Raymond, John, Fox, Ori D., Modjaz, Maryam, Spitkovsky, Anatoly, Strolger, Lou
We present JWST observations of the Crab Nebula, the iconic remnant of the historical SN 1054. The observations include NIRCam and MIRI imaging mosaics, plus MIRI/MRS IFU spectra that probe two select locations within the ejecta filaments. We derive
Externí odkaz:
http://arxiv.org/abs/2406.00172
Autor:
Lyutikov, Maxim
We provide an overview of various mechanisms, and corresponding powers, of precursor emission to compacts' mergers to be detected by LIGO-Virgo-KAGRA (LVK) collaboration. Expected peak powers, $\leq 10^{43}$ erg s$^{-1}$, are not sufficiently high to
Externí odkaz:
http://arxiv.org/abs/2402.16504
Autor:
Pelisoli, Ingrid, Sahu, Snehalata, Lyutikov, Maxim, Barkov, Maxim, Gaensicke, Boris T., Brink, Jaco, Buckley, David A. H., Potter, Stephen B., Schwope, Axel, Ramirez, S. H.
J191213.72-441045.1 is a binary system composed of a white dwarf and an M-dwarf in a 4.03-hour orbit. It shows emission in radio, optical, and X-ray, all modulated at the white dwarf spin period of 5.3 min, as well as various orbital sideband frequen
Externí odkaz:
http://arxiv.org/abs/2311.05558
Autor:
Lower, Marcus E., Johnston, Simon, Lyutikov, Maxim, Melrose, Donald B., Shannon, Ryan M., Weltevrede, Patrick, Caleb, Manisha, Camilo, Fernando, Cameron, Andrew D., Dai, Shi, Hobbs, George, Li, Di, Rajwade, Kaustubh M., Reynolds, John E., Sarkissian, John M., Stappers, Benjamin W.
Radio emission from magnetars provides a unique probe of the relativistic, magnetized plasma within the near-field environment of these ultra-magnetic neutron stars. The transmitted waves can undergo birefringent and dispersive propagation effects th
Externí odkaz:
http://arxiv.org/abs/2311.04195
Autor:
Lyutikov, Maxim, Freund, Henry
Using the ONEDFEL code we perform Free Electron Laser simulations in the astrophysically important guide-field dominated regime. For wigglers' (Alfven waves) wavelengths of tens of meters and beam Lorentz factor $\sim 10^3$, the resulting coherently
Externí odkaz:
http://arxiv.org/abs/2310.17028
Autor:
Lyutikov, Maxim
We reconsider the escape of high brightness coherent emission of Fast Radio Bursts (FRBs) from magnetars' magnetospheres, and conclude that there are numerous ways for the powerful FRB pulse to avoid nonlinear absorption. Sufficiently strong surface
Externí odkaz:
http://arxiv.org/abs/2310.01177
Autor:
Lyutikov, Maxim, Ibrahim, Ahmad
We point out the dominant importance of plasma injection effects for relativistic winds from pulsars and black holes. We demonstrate that outside the light cylinder the magnetically dominated outflows while sliding along the helical magnetic field mo
Externí odkaz:
http://arxiv.org/abs/2305.09879
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 524, Issue 4, October 2023, Pages 6024-6051
We study dynamics of relativistic Coronal Mass Ejections (CMEs), from launching by shearing of foot-points (either slowly - the ``Solar flare'' paradigm, or suddenly - the ``star quake" paradigm), to propagation in the preceding magnetar wind. For sl
Externí odkaz:
http://arxiv.org/abs/2302.08848
Autor:
Lyutikov, Maxim
We first derive a set of equations describing general stationary configurations of relativistic force-free plasma, without assuming any geometric symmetries. We then demonstrate that electromagnetic interaction of merging neutron stars is necessarily
Externí odkaz:
http://arxiv.org/abs/2211.14433
In gamma-ray binaries neutron star is orbiting a companion that produces a strong stellar wind. We demonstrate that observed properties of "stellar wind"-"pulsar wind" interaction depend both on the overall wind thrust ratio, as well as more subtle g
Externí odkaz:
http://arxiv.org/abs/2211.12053