Results 161 to 170 of about 10,429 (199)

Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]

Space Sci Rev
Liu YH, Hesse M, Genestreti K, Nakamura R, Burch JL, Cassak PA, Bessho N, Eastwood JP, Phan T, Swisdak M, Toledo-Redondo S, Hoshino M, Norgren C, Ji H, Nakamura TKM.   +14 more
europepmc   +1 more source

Extended main sequences in star clusters. [PDF]

Fundam Res
Li C, Milone AP, Sun W, de Grijs R.
europepmc   +1 more source

Magnetars [PDF]

Annual Review of Astronomy and Astrophysics, 2017
Magnetars are young and highly magnetized neutron stars that display a wide array of X-ray activity including short bursts, large outbursts, giant flares, and quasi-periodic oscillations, often coupled with interesting timing behavior including enhanced spin-down, glitches, and antiglitches.
Andrei M Beloborodov
exaly   +5 more sources

The early evolution of magnetar rotation – I. Slowly rotating ‘normal’ magnetars

Monthly Notices of the Royal Astronomical Society, 2022
ABSTRACT In the seconds following their formation in core-collapse supernovae, ‘proto’-magnetars drive neutrino-heated magnetocentrifugal winds. Using a suite of two-dimensional axisymmetric magnetohydrodynamic simulations, we show that relatively slowly rotating magnetars with initial spin periods of P⋆0 = 50–500 ms spin down rapidly ...
Tejas Prasanna, Matthew S B Coleman, Matthias J Raives   +2 more
exaly   +3 more sources

Pulse frequency fluctuations of magnetars [PDF]

Monthly Notices of the Royal Astronomical Society, 2019
18 pages, 1 table, 4 figures, accepted for publication in ...
Cerri-Serim, D., Serim, M. M., Sahiner, S., Inam, S. C., Baykal, A.   +4 more
exaly   +4 more sources

Some of the next articles are maybe not open access.

Related searches:

Nature of ``Magnetars"

Chinese Journal of Astronomy and Astrophysics, 2006
A brief review of known models for the description of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Repeaters (SGRs) is given. A new model is proposed to explain the main properties of these objects and radio pulsars with long periods on the base of the conception of drift waves in the vicinity of the light cylinder of the neutron star with the ...
I. F Malov, G. Z Machabeli
openaire   +1 more source

Observations of Magnetars

AIP Conference Proceedings, 2008
The salient properties of magnetars are summarized here with an emphasis on recent developments in the field since 2005. In particular, I discuss observations of the giant flares, bursts from Anomalous X‐ray Pulsars (AXPs), transient emission from AXPs, multi‐wavelength observations of magnetars, glitch activity in AXPs, magnetar energy spectra, and ...
Peter M. Woods, C. Bassa, Z. Wang, A. Cumming, V. M. Kaspi   +4 more
openaire   +1 more source

Diventerà una magnetar

2023
Scoperta di recente, Hd 45166, una stella massiccia con un campo magnetico di 43mila gauss (il più forte mai trovato in una stella di massa elevata), secondo gli astronomi potrebbe terminare la sua vita come magnetar. Man mano che la stella collasserà su sé stessa, infatti, il suo campo magnetico si rafforzerà e Hd 45166 finirà per diventare un ...
openaire   +1 more source

L’imprevedibilità delle magnetar

2023
A distanza di oltre tre anni dal 28 aprile 2020, un team internazionale di scienziati riferisce l’esito delle osservazioni effettuate con il radiotelescopio cinese Fast del primo lampo radio veloce galattico, riportando di aver scoperto una fase di pulsar radio della magnetar che lo ha emesso.
openaire   +1 more source