The blueshift of the 發(fā)射譜線窄線藍(lán)移的項目管理辦公室

1、the blueshift of the o iii emission line in nls1soutline1. introduction: nls1s, m- observation: narrow theory: less massive black hole higher eddington ratio early stage of agn evolution 1. introduction150 nls1s from sdss edr (williams r.j., pogge r.w., mathur s, 2003, aj, 124, 3042)22 nls1s from hs

2、t observation(constantin & shields, 2003, pasp, 115, 592)1.2 m relation in nls1s (bian & zhao, mnras, 2004, 347, 607; grupe & mathur, 2004, apj, 606, l41;botte, 2005, mnras, 356, 789)dynamics of nlrs in nls1s would be different than that of other agn216 low-redshift agn(zamanzov r., et a

3、l., 2002, apj, 576, l9)two largest blueshift of o iii (aoki k., et al., 2005, apj, 618, 601)1.3 the shift of the peak of o iii relative to hthe o iii blueshift versus the fwhm(h), and fe ii4570/ hin the population a region of the eigenvector 1 parameter domain= strong fe ii lines and narrow h linere

4、f:boroson t. a., oke j. b., 1987, pasp, 99, 809grupe d., thomas h.-c., leighly k. m., 2001, a&a, 369, 450veron-cetty m.-p., veron, p., goncalves a. c., 2001, a&a, 372, 730grupe d., leighly k. m. 2002, in x-ray spectroscopy of agn with chandra and xmm-newton, ed. t. boller (mpe rep. 279; garc

5、hing: mpe), 287zamanzov r., et al., 2002, apj, 576, l9 marziani p., et al., 2003, mnras, 345, 1133aoki k., kawaguchi t., ohtack., 2005, apj, 618, 6012. sdss sample and analysis150 nls1 in sdss edriraf-specfit: correct the blue wind of o iii (1) a power-law continuum (2) fe ii multiples (3) three two-component sets for h 3.1 distributions of the blueshift3.2 the “blue outliers”for sdss j0102226.31-003904.6:criterion:for sdss j024037.89+001118.9:3.3 correlations between the blueshift andsome parameters4. summarytwo-compo