2014ApJ...781L..10W


Query : 2014ApJ...781L..10W

2014ApJ...781L..10W - Astrophys. J., 781, L10 (2014/January-3)

A double neutron star merger origin for the cosmological relativistic fading source PTF11agg?

WU X.-F., GAO H., DING X., ZHANG B., DAI Z.-G. and WEI J.-Y.

Abstract (from CDS):

The Palomar Transient Factory (PTF) team recently reported the discovery of a rapidly fading optical transient source, PTF11agg. A long-lived scintillating radio counterpart was identified, but the search for a high-energy counterpart showed negative results. The PTF team speculated that PTF11agg may represent a new class of relativistic outbursts. Here we suggest that a neutron star (NS)-NS merger system with a supra-massive magnetar central engine could be a possible source to power such a transient, if our line of sight is not on the jet axis direction of the system. These systems are also top candidates for gravitational wave sources to be detected in the advanced LIGO/Virgo era. We find that the PTF11agg data could be explained well with such a model, suggesting that at least some gravitational wave bursts due to NS-NS mergers may be associated with such a bright electromagnetic counterpart without a γ-ray trigger.

Abstract Copyright: ∼

Journal keyword(s): gravitational waves - radiation mechanisms: non-thermal - stars: neutron

Simbad objects: 2

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Number of rows : 2
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 PTF 11agg SN* 08 22 17.195 +21 37 38.26           ~ 31 0
2 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0

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