GRB 210610B: The Internal and External Plateau as Evidence for the Delayed Outflow of Magnetar
After launching a jet, outflows of magnetar were used to account for the achromatic plateau of afterglow and the early X-ray flux plateau known as “internal plateau”. The lack of detecting magnetic dipole emission together with the energy injection feature in a single observation poses confusion unt...
Gespeichert in:
Veröffentlicht in: | Research in astronomy and astrophysics 2024-07, Vol.24 (7), p.75013 |
---|---|
Hauptverfasser: | , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | After launching a jet, outflows of magnetar were used to account for the achromatic plateau of afterglow and the early X-ray flux plateau known as “internal plateau”. The lack of detecting magnetic dipole emission together with the energy injection feature in a single observation poses confusion until the long gamma-ray burst (GRB) 210610B is detected. GRB 210610B is presented with an optical bump following an early X-ray plateau during the afterglow phase. The plateau followed by a steep decline flux overlays in the steadily decaying X-ray flux with index
α
X,1
∼ 2.06, indicating an internal origin and that can be fitted by the spin-down luminosity law with the initial plateau luminosity
log
10
L
X
∼
48.29
erg
s
−
1
and the characteristic spin-down timescale
T
∼ 2818 s. A subsequent bump begins at ∼4000 s in the
R
band with a rising index
α
R,1
∼ − 0.30 and peaks at ∼14125 s, after which a decay index
α
R,2
∼ 0.87 and finally transiting to a steep decay with
α
R,3
∼ 1.77 achieve the closure relation of the external shock for the normal decay phase as well as the magnetar spin-down energy injection phase, provided that the average value of the photon index Γ
γ
= 1.80 derived from the spectral energy distributions (SEDs) between the X-ray and optical afterglow. The closure relation also works for the late X-ray flux. Akin to the traditional picture of GRB, the outflow powers the early X-ray plateau by dissipating energy internally and collides with the leading decelerating blast burst as time goes on, which could interpret the exotic feature of GRB 210610B. We carry out a Markov Chain Monte Carlo simulation and obtain a set of best parameters:
ϵ
B
≃ 4.7 × 10
−5
,
ϵ
e
≃ 0.15,
E
K,iso
≃ 4.6 × 10
53
erg, Γ
0
≃ 832,
A
*
≃ 0.10,
L
inj,0
≃ 3.55 × 10
50
erg s
−1
. The artificial light curve can fit the afterglow data well. After that, we estimated the average Lorentz factor and the X-ray radiation efficiency of the later ejecta are 35% and 0.13%, respectively. |
---|---|
ISSN: | 1674-4527 2397-6209 |
DOI: | 10.1088/1674-4527/ad4d3a |