TXS 1433+205: The most distant gamma-ray emitting FR II radio galaxy

被引:1
|
作者
Paliya, Vaidehi S. [1 ]
Saikia, D. J. [1 ]
Stalin, C. S. [2 ]
机构
[1] Interuniv Ctr Astron & Astrophys IUCAA, SPPU Campus, Pune 411007, India
[2] Indian Inst Astrophys, Block 2,Koramangala, Bengaluru 560034, Karnataka, India
基金
加拿大创新基金会;
关键词
BL Lacertae objects: general; galaxies: jets; gamma-rays: galaxies; AREA TELESCOPE OBSERVATIONS; ACTIVE GALACTIC NUCLEI; DATA RELEASE; SKY SURVEY; FERMI-LAT; QUASARS; POPULATION; CATALOG; DEPOLARIZATION; SPECTROSCOPY;
D O I
10.1093/mnrasl/slac165
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The orientation of the jet axis to the line of sight of the observer plays a major role in explaining the phenomena observed from blazars and radio galaxies. In the.-ray band, only a handful of radio galaxies have been identified, all being located in the nearby Universe (z < 0.5). Here, we report the identification of 4FGL J1435.5+2021, associated with TXS 1433+205, as a Fanaroff-Riley type II (FR II) radio galaxy at a considerably higher redshift of z = 0.748, thereby making it the most distant gamma-ray detected radio galaxy known as of now. The Very Large Array Sky Survey data at 3 GHz resolves the source morphology into a bright core, a jet and two hotspots, with a total end-to-end projected length between lobe extremities of similar to 170 kpc. The optical and radio properties of this enigmatic object suggest it to be a high-excitation FR II radio galaxy. The multiwavelength behaviour of TXS 1433+205 is found to be similar to other gamma-ray detected FR II sources but is at the high-luminosity end. We suggest that the ongoing and upcoming high-resolution radio surveys will lead to the identification of many more high-redshift radio galaxies in the gamma-ray sky, thus allowing comprehensive studies of misaligned relativistic jets.
引用
收藏
页码:L33 / L37
页数:5
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