'Ir qsos' presentation slideshows

From ULIRGs to QSOs

From ULIRGs to QSOs. XiaoYang, Xia Center for Astrophysics Tianjin Normal University Collaborators: H. Wu, Deng, Zou, Z. Zheng, Mao, X.Z. Zheng, Hao, Huo, Y. Gao, Wang,J.L, Tan. Outline. The morphology and environment of ULIRGs and LIRGs May give hint for high-z SMGs

1.37k views • 118 slides

Surveys of high-z galaxies and galaxy clusters with AzTEC

863 views • 72 slides

Mid- Infrared Spectroscopic Properties of IR QSOs

Mid- Infrared Spectroscopic Properties of IR QSOs. XiaoYang, Xia Center for Astrophysics Tianjin Normal University. Outline. Infrared Luminous QSOs (IR QSO) Spitzer IRS Spectra of IR QSOs.

782 views • 65 slides

IR QSOs at low and high redshift

IR QSOs at low and high redshift. X.Y.Xia Tianjin Normal University, China Collaborators: C.N.Hao, S.Mao, H.Wu & Z.G.Deng. Motivation. The tight correlation between Mbh and ? of host galaxy Kommendy&Gebhardt 2001, Merritt & Ferrarese 2001 The relation of SFR/Mdot vs. Mbh

556 views • 44 slides

The Coeval Growth of Black Holes and their host Spheriods

The Coeval Growth of Black Holes and their host Spheriods. X.Y.Xia Tianjin Normal University, China Collaborators: C.N.Hao, S.Mao, Z.G.Deng &H.Wu. Motivation. The tight correlation between Mbh and the mass of host spheriod Kommendy&Gebhardt 2001, Merritt & Ferrarese 2001

394 views • 32 slides