TAURUS observations of the [O III] cone in NGC 1068
نویسندگان
چکیده
منابع مشابه
VLTI/VINCI observations of the nucleus of NGC 1068 using the adaptive optics system MACAO
We present the first near-infrared K-band long-baseline interferometric measurement of the nucleus of the prototype Seyfert 2 Galaxy NGC 1068 with resolution λ/B ∼ 10 mas obtained with the Very Large Telescope Interferometer (VLTI) and the two 8.2 m diameter Unit Telescopes UT 2 and UT 3. The adaptive optics system MACAO (Multi Application Curvature Adaptive Optics) was employed to deliver wave...
متن کاملSlow Jets in Seyfert Galaxies : NGC 1068
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany 2 Department of Astronomy, University of Maryland, College Park, MD 20742, USA 3 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 4 National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801, USA 5 Johns Hopkins University, Department of Physics and Astronomy, Homewood Cam...
متن کاملA new analysis of the nucleus of NGC 1068 with MIDI observations
We present a new analysis of the very first mid-infrared N-band long-baseline interferometric observations of an extragalactic source: the nucleus of the Seyfert 2 galaxy NGC 1068, obtained with MIDI (Mid-InfrareD Interferometer), the mid-infrared beamcombiner at the European Southern Observatory (ESO) Very Large Telescope Interferometer (VLTI). The resolution of λ/B = 10 mas allows to study th...
متن کاملTesting the Seyfert unification theory : Chandra HETGS observations of NGC 1068
We present spatially resolved Chandra HETGS observations of the Seyfert 2 galaxy NGC 1068. Xray imaging and high resolution spectroscopy are used to test the Seyfert unification theory. Fe Kα emission is concentrated in the nuclear region, as are neutral and ionized continuum reflection. This is consistent with reprocessing of emission from a luminous, hidden X-ray source by the obscuring molec...
متن کاملISO - SWS spectroscopy of NGC 1068
We present ISO-SWS spectroscopy of NGC 1068 for the complete wavelength range 2.4 to 45μm at resolving power ∼1500. Selected subranges have been observed at higher sensitivity and full resolving power ∼2000. We detect a total of 36 emission lines and derive upper limits for 13 additional transitions. Most of the observed transitions are fine structure and recombination lines originating in the ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1992
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/258.2.371