Compact Steep Spectrum Radio Sources with Enhanced Star Formation Are Smaller Than 10 kpc

被引:5
作者
Gordon, Yjan A. [1 ]
O'Dea, Christopher P. [2 ]
Baum, Stefi A. [2 ]
Bechtol, Keith [1 ]
Duggal, Chetna [2 ]
Ferguson, Peter S. [1 ]
机构
[1] Univ Wisconsin Madison, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
[2] Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会; 美国国家航空航天局;
关键词
ACTIVE GALACTIC NUCLEI; GHZ PEAKED SPECTRUM; FORMATION HISTORIES; VLBI OBSERVATIONS; SYMMETRIC OBJECT; FORMING GALAXIES; MINOR MERGERS; SKY; EVOLUTION; ASTROPY;
D O I
10.3847/2041-8213/accf0a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Compact steep spectrum (CSS) radio sources are active galactic nuclei (AGN) that have radio jets propagating only on galactic scales, defined as having projected linear size (LS) of up to 20 kpc. CSS sources are generally hosted by massive early-type galaxies with little ongoing star formation; however, a small fraction are known to have enhanced star formation. Using archival data from the Faint Images of the Radio Sky at Twenty cm survey, the Very Large Array Sky Survey, and the Sloan Digital Sky Survey, we identify a volume-limited sample of 166 CSS sources at z < 0.2 with L (1.4 GHz) > 10(24) W Hz(-1). Comparing the star formation rates and linear sizes of these CSS sources, we find that the approximate to 14% of CSS sources with specific star formation rates above 0.01 Gyr(-1) all have LS < 10 kpc. We discuss the possible mechanisms driving this result, concluding that it is likely the excess star formation in these sources occurred in multiple bursts and ceased prior to the AGN jet being triggered.
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页数:7
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