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《天文和天体物理学研究(英文版)》 2015-06
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The inner~40 pc radial distribution of the star formation rate for a nearby Seyfert 2 galaxy M51

Li-Ling Fang;Xiao-Lei Jiang;Zhi-Cheng He;Wei-Hao Bian;Department of Physics and Institute of Theoretical Physics, Nanjing Normal University;  
We investigate the spatially resolved specific star formation rate(SSFR)in the inner ~40 pc for a nearby Seyfert 2 galaxy, M51(NGC 5194) by analyzing spectra obtained with the Hubble Space Telescope(HST) Space Telescope Imaging Spectrograph(STIS). We present 24 radial spectra measured along the STIS long slit in M51, extending ~ 1′′from the nucleus(i.e., –41.5 pc to 39.4 pc). By simple stellar population synthesis, the stellar contributions in these radial optical spectra are modeled. It is found that the mean flux fraction of young stellar populations(younger than24.5 Myr) is about 9%. Excluding some regions with zero young flux fraction near the center(from –6 pc to 2 pc), the mean mass fraction is about 0.09%. The young stellar populations are not required in the center inner ~8 pc in M51, suggesting a possible SSFR suppression in the circumnuclear region(~ 10 pc) from the feedback of active galactic nuclei(AGNs). The radial distribution of SSFR in M51 is not symmetrical with respect to the long slit in STIS. This unsymmetrical SSFR distribution is possibly due to the unsymmetrical AGN feedback in M51, which is related to its jet.
【Fund】: Supported by the National Natural Science Foundation of China
【CateGory Index】: P152
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【Co-citations】
Chinese Journal Full-text Database 2 Hits
1 YUAN Qi-rong;ZHAO Zhen-yu;JING Wei;XU Hao-jie;School of Physics Science and Technology,Nanjing Normal University;;The Star Formation History of Galaxy Cluster Abell 85[J];Acta Astronomica Sinica;2013-05
2 Zhi-Min Zhou;Hong Wu;Lei Huang;Hong-Bin Li;Zhi-Zhong Zhou;Jun-Jun Jia;Man-I Lam;Yi-Nan Zhu;Key Laboratory of Optical Astronomy, National Astronomical Observatories,Chinese Academy of Sciences;Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences;;Metallicity and star formation activities of the interacting system Arp 86 from observations with MOS on the Xinglong 2.16m telescope[J];天文和天体物理学研究(英文版);2014-11
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