2024MNRAS.529.4287S


Query : 2024MNRAS.529.4287S

2024MNRAS.529.4287S - Mon. Not. R. Astron. Soc., 529, 4287-4294 (2024/April-3)

Revisiting the time-integrated polarizations of gamma-ray burst prompt phase.

SUI L.-Q. and LAN M.-X.

Abstract (from CDS):

In previous studies, the time evolution information is missed in deducing the time-integrated polarizations of gamma-ray burst prompt emission. Here, it is considered and the time-integrated polarizations is investigated through the summation of the time-resolved ones. The statistical properties of the distribution of the time-integrated polarization degree (Π) can be read from the q-Π curve, where q ≡ θV/θj. θV and θj are the observational and jet half-opening angles, respectively. Hence, only the q-Π curves are studied. In addition to a toroidal magnetic field in the radiation region, an aligned field is also discussed. We found the predicted time-integrated polarization degree is around $(40\!-\!50)\,\, \mathrm{ per\,cent}$ for High-energy Polarimetry Detector (HPD) onboard POLAR-2 and is roughly $(30\!-\!40)\,\, \mathrm{ per\,cent}$ for its Low-energy Polarimetry Detector (LPD). Therefore, Π value detected by the HPD will be larger than that of the LPD in statistics and the result of the former estimations will underestimate the value of Π in an ordered field. There are mainly two types of the q-Π curve profiles, corresponding to two ordered magnetic field configurations.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): magnetic fields - gamma-ray bursts - polarization - radiation mechanisms: non-thermal - magnetic reconnection - stars: jets

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Fermi bn170114917 gB 00 48 -12.6           ~ 36 0

Query : 2024MNRAS.529.4287S

Basic data :
Fermi bn170114917 -- Gamma-ray Burst
Other object types:
otypes_help
gB (2020ApJ,GRB,...)
ICRS coord. (ep=J2000) :
00 48 24.0 -12 36 00 (Gamma-ray) [ 3600000 3600000 90 ] E 2020ApJ...893...46V
FK4 coord. (ep=B1950 eq=1950) :
00 45 53.3 -12 52 21 [ 3600000 3600000 90 ]
Gal coord. (ep=J2000) :
119.9796 -75.4543 [ 3600000 3600000 90 ]
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon

Identifiers (2) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

GRB 170114A Fermi bn170114917

References (36 between 1850 and 2026) (Total 36)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2024MNRAS.529.4287S and select 'bookmark this link' or equivalent in the popup menu