Infrared spectroscopy of nearby radio active early-type galaxies-II: spectral atlas

被引:0
|
作者
Durre, Mark [1 ]
Mould, Jeremy [1 ]
Brown, Michael [2 ]
Reynolds, Tristan [3 ,4 ]
机构
[1] Swinburne Univ, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[2] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia
[3] Univ Western Australia, Int Ctr Radio Astron Res ICRAR, 35 Stirling Highway, Crawley, WA 6009, Australia
[4] ARC Ctr Excellence All Sky Astrophys 3 Dimens ASTR, Fremantle, WA, Australia
基金
美国安德鲁·梅隆基金会; 美国国家科学基金会; 美国国家航空航天局;
关键词
galaxies: elliptical and lenticular; cD; infrared: general; radio continuum: galaxies; galaxies: active; galaxies: nuclei; INTEGRAL FIELD SPECTROSCOPY; GEMINI NIFS SURVEY; GALACTIC NUCLEI; FE-II; MOLECULAR-HYDROGEN; LINE REGION; FEEDBACK; EMISSION; GAS; AGN;
D O I
10.1093/mnras/stad2083
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a near-infrared spectroscopic atlas of nearby, bright early-type galaxies with radio emission, containing 163 galaxies observed by the Palomar 200'' TripleSpec instrument, measuring the emission line fluxes for H, He, [Fe II], and H-2 and determined the nuclear excitation mechanisms. By stacking spectra, we deduced the H-2 excitation temperature (1957 +/- 182 K) and dominant excitation mechanism (thermal and shock heating combined) from the K-band emission line sequence. Stacking also produces an 'average' spectrum of absorption features and spectral indices from the literature; the CO12 absorption line index versus J - K colour shows a trend of stronger nuclear activity producing a weaker CO12 index and a redder (flatter) continuum. The correlations between the radio and the emission-line luminosities finds a trend with radio power; however, the large scatter in the upper limits shows that the two are not directly coupled and the duty cycles of SF and AGN activity are not synchronized.
引用
收藏
页码:4923 / 4938
页数:16
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