The ionized gas in this region forms a spiral pattern (see e.g. Lo & Claussen ... The western side of this feature represents the inner edge of a large ring of ...
(1)OAN- Observatorio Astronomico Nacional, Madrid, Spain(2) LERMA, Observatoire ... The variety of morphologies of circumnuclear gas disks is remarkably large: ...
The problem: How is the activity of MBHs decreased/switched off after the bright ... available: stellar mass losses steadily replenishing the circumnuclear region. ...
Black Hole Feeding & Feedback: what can we learn from nearby AGN? Richard Davies, Eckhard Sturm Max Planck Institute for Extraterrestrial Physics, Germany
Molecular absorption in. Cen A on VLBI scales. Huib Jan van Langevelde, JIVE. Ylva Pihlstr m, NRAO ... The physical and chemical properties of starburst ...
X-ray spectroscopy of bright Seyfert 2s: The importance of the 10 ... Harvard-Smithsonian Center for Astrophysics. One Case study: XMM observations of NGC 1365 ...
The stacked spectrum of all the objects with good SNR included in CIELO confirms ... lines) are also recovered in the stacked spectrum of poor SNR objects (~60 ...
Consider the Circinus galaxy... Jones et al. (1999) Veilleux ... In Circinus, conditions. support H2O masers in. an edge-on accretion disk. a nuclear outflow ...
... lie in a ring of radius. r~22pc. Velocity field confirms ... Spectral index map using 1.3 Global VLBI and 5 GHz VLBA observations. free-free optical depth: ...
(vorticity in the axisymmetric flow flield has a local extremum) ... We believe that the origin of the shear instability lies on the vorticity creation on shocks. ...
UN ESTUDIO DE ESCENARIOS INESTABLES EN LA GALAXIA NGC 5427. Vlad mir Jearim PE A-SU REZ, F s. ... Sy II espiral de dos brazos con extensas ... (Combes, 2000) ...
Exploring structure around submillimetre-bright QSOs Francisco J. Carrera (IFCA, CSIC-UC, Spain/Imperial, UK) Mathew J. Page (MSSL-UCL, UK) Jason Stevens (CAR, U ...
Class of AGN consisting of BL Lac objects and gamma-ray bright quasars ... Qe,p (g,t) g. Synchrotron emission of primary e- nFn. n. Proton-induced radiation ...
Local ioniz. ... Cross correlation in channels, or 3D power spectrum ... Enrichment of heavy elements, dust starts early (z 8): good news for radio astronomy ...
Both studies are unique in that they probe the very central regions of galaxies, ... 1) The Central 10 Parsec of Sb-S0 bulges are in ~80% of the cases dominated by ...
Stacked spectra technique, trend of Fe line intensity with physical quantities of the sources ... Fe K transitions give rise to prominent fluorescence lines in ...
Robert Sharp and Stuart Ryder AAO Johan Knapen U. Hertfordshire Lisa Mazzuca GSFC Ian Parry U. Cambridge Integral field spectroscopy in the IR: Gemini-CIRPASS ...
KNAW colloquium 'Cosmic Voids' December 12-15, 2006 ... I. Void Finding in Nearby Redshift Surveys. Fiona Hoyle, Danny Pan ... Anca Constantin, Fiona Hoyle ...
STAR FORMATION RATE E MORFOLOGIA DELLE GALASSIE formazione stellare tecniche osservative correlazioni morfologiche Simone Callegari, Esame di Astronomia ...
... with H.-W. Rix, J. Shields, A. Barth, L. Ho, A. Filippenko, W. Sargent, G. ... Both studies are unique in that they probe the very central regions of galaxies, ...
Review of High Energy Astrophysics Research in Mainland China Zhang, Shuang Nan Tsinghua Center for Astrophysics (THCA) and Physics Department Tsinghua University ...
High Angular Resolution Imaging of the Galactic Center Andrea Ghez University of California Los Angeles Collaborators E. E. Becklin, G. Duchene, S. Hornstein, J. Lu ...
Different light production mechanisms dominate portions of galaxies spectra and ... Only with a combination of Optical (HST), X-Ray (Chandra), Thermal IR (SIRTF) ...
* * * * * PSU group results (CV, Steffen, Just, Gibson)+Young+10 but see earlier Einstein results Lusso+10 for X-ray selected see poster by Antonucci Properties ...
Open questions: relative contribution SB and AGN. Need of observation above 10 keV ... To calibrate a SFR IR-X ray indicator is fundamental a direct measure of the ...
Dmitry Sokoloff, Vladimir Shoutenkov (Moscow) Peter Frick, Igor Patrickeyev (Perm) ... Halo fields (see next talk by Ralf-J rgen Dettmar) Observation of ...
The active nucleus in Seyfert 2 (and by extension other low ... i.- We characterize the young, massive stellar population from. the analysis of the UV continuum. ...
Only few examples of X-ray bright BLRGs at low z and with an optimal inclination ... 5 lines clearly detected with the EPIC-CCD: OVII He- , OVIII Ly , MgXI and SiXIII ...
deep Ha, UV imaging of volume-complete 11 Mpc samples - Spitzer followup proposed ... Ha imaging followup of Arecibo ALFALFA HI survey. Fourth Generation: blind ...
... type galaxy with SF activity in the Virgo cluster ... along the CM relation in Virgo Cluster (PID 3419 cycle 1 - PI ... with MIR signs of SF activity: ...
XMM-Newton observations of many other bright Seyfert galaxies, however, found ... (or moderately obscured) AGN publicly available in the XMM-Newton archive. ...
Thin disks, H/R 0.1, optically thick, emit the ' Big Blue Bump ' Seyfert ... with galaxy bulges, and a fraction of elliptical galaxies (large bulges) are due ...