Qingwen Wu

Details der Publikationsliste

Zeitraum

2004 - 2009

Anzahl

12

Co-Autoren

Estimation of Magnetic Field Strength in the Turbulent Warm Ionized Medium (2009)

Wu, Qingwen, Kim, Jongsoo, Ryu, Dongsu, Cho, Jungyeon, Alexander, Paul

We studied Faraday rotation measure (RM) in turbulent media with the rms Mach number of unity, using isothermal, magnetohydrodynamic turbulence simulations. Four cases with different values of...

Accretion/Jet Activity and Narrow [O III] Kinematics in Young Radio Galaxies (2009)

Wu, Qingwen, Gu, Minfeng, Humphrey, Andrew

We estimate black hole masses and Eddington ratios for a sample of 81 young radio galaxies (42 CSS +39 GPS). We find that the average black hole (BH) mass of these young radio galaxies is ~8.3, which...

Observational Evidence for Young Radio Galaxies are Triggered by Accretion Disk Instability (2009)

Wu, Qingwen

The bolometric luminosities and black hole (BH) masses are estimated by various methods for a sample of young radio galaxies with known ages. We find that the ages are positively correlated with the...

The black hole mass, Eddington ratio, and M_bh-\sigma_[O III] relation in young radio galaxies (2009)

Wu, Qingwen

The BH masses and the Eddington ratios for a sample of 65 young radio galaxies [27 GPS and 38 CSS sources] are estimated by various methods. We find that the average BH mass of these young radio...

On the BL Lacertae objects/radio quasars and the FRI/II dichotomy (2009)

Xu, Ya-Di, Cao, Xinwu, Wu, Qingwen

In the frame of unification schemes for radio-loud active galactic nuclei (AGNs), FR I radio galaxies are believed to be BL Lacertae (BL Lac) objects with the relativistic jet misaligned to our line...

The Hard X-ray Spectral Evolution in XRBs, AGNs and ULXs (2008)

Wu, Qingwen, Gu, Minfeng

We explore the relationship between the hard X-ray photon index $\Gamma$ and the Eddington ratio (\xi=L_{X}(0.5-25 keV)/L_{Edd}) in six XRBs. We find that different XRBs follow different...

Origin of the X-ray Emission in the Nuclei of FR Is (2008)

Wu, Qingwen, Yuan, Feng, Cao, Xinwu

We investigate the X-ray origin in FRIs using the multi-waveband high resolution data of eight FR I sources, which have very low Eddington ratios. We fit their multi-waveband spectrum using a coupled...

Jet power extracted from ADAF and the applications to X-ray binaries and radio galaxy FR dichotomy (2008)

Wu, Qingwen, Cao, Xinwu

We calculate the jet power of the classical Blandford-Znajek(BZ) model and hybrid model developed by Meier based on the global solutions of advection dominated accretion flows (ADAFs) surrounding...

The hard X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources (2008)

Wu, Qingwen, Gu, Minfeng

We investigate the relationship between the hard X-ray photon index $\Gamma$ and the Eddington ratio ($\xi=L_{X}(0.5-25 \rm keV)/L_{Edd}$) in six X-ray binaries (XRBs) with well constrained black...

On the origin of X-ray emission in some FR Is: ADAF or jet? (2007)

Wu, Qingwen, Yuan, Feng, Cao, Xinwu

We investigate the X-ray origin in FR Is using the radio, submillimetre, optical, and {\em Chandra} X-ray data of a small sample consisting of eight FR I sources. These sources are very dim, with...

The relation between star formation rate and accretion rate in LINERs (2006)

Wu, Qingwen, Cao, Xinwu

It is argued that there is a linear correlation between star formation rate (SFR) and accretion rate for normal bright active galactic nuclei (AGNs). However, it is still unclear whether this...

Origin of Radio Emission from Nearby Low-Luminosity Active Galactic Nuclei (2004)

Wu, Qingwen, Cao, Xinwu

We use the observational data in radio, optical and X-ray wavebands, for a sample of active galactic nuclei (AGNs) with measured black hole masses, to explore the origin of radio emission from nearby...