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Related papers: Silicate absorption in heavily obscured galaxy nuc…

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We report a detection of the 9.7 micrometer silicate absorption feature in a damped Lyman-alpha (DLA) system at z_{abs} = 0.524 toward AO0235+164, using the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. The feature shows…

Astrophysics · Physics 2009-06-23 Varsha P. Kulkarni , Donald G. York , Giovanni Vladilo , Daniel E. Welty

We present K-band spectroscopy for several regions of three nearby spiral galaxies, NGC 613, NGC 628 and NGC 7741. Analysis of the depth of the 2.293 micron CO absorption feature in these spectra reveals that some regions have deep…

Astrophysics · Physics 2007-05-23 P. A. James , M. S. Seigar

We report the Rossi X-ray Timing Explorer observations of the heavily absorbed Seyfert 2 galaxy NGC 4945, which confirm the large column density of the absorber, corresponding to the optical depth to Thomson scattering of about 2.4. The…

Astrophysics · Physics 2009-10-31 G. M. Madejski , P. T. Zycki , C. Done , A. Valinia , P. Blanco , R. Rothschild , B. Turek

Absorption-line spectroscopy of 23 background QSOs and numerous background galaxies has let us measure the spatial distribution of metals and neutral hydrogen around 1044 UV-selected galaxies at redshifts 1.8<z<3.3. The typical galaxy is…

Astrophysics · Physics 2008-11-26 K. L. Adelberger , A. E. Shapley , C. C. Steidel , M. Pettini , D. K. Erb , N. A. Reddy

We present observations of the intrinsic absorption in the Seyfert 1 galaxy NGC 3783 obtained with the STIS/HST and FUSE. We have coadded multiple STIS and FUSE observations to obtain a high S/N averaged spectrum spanning 905-1730 A. The…

The intervening z=0.7443 Mg II absorption system in the spectrum of MC 1331+170 shows an unusual series of line pairs, each with velocity separations of 30 km/s. These lines could be explained as the shells of expanding superbubbles…

Astrophysics · Physics 2009-11-06 Nicholas A. Bond , Chris W. Churchill , Jane C. Charlton , Steven S. Vogt

We study the absorption and scattering of X-ray radiation by interstellar dust particles, which allows us to access the physical and chemical properties of dust. The interstellar dust composition is not well understood, especially on the…

Spectra that cover wavelengths from 0.6 to 1.1um are used to examine the behavior of emission and absorption features in a contiguous 22 x 300 arcsec region centered on the nearby dwarf galaxy NGC 55. Based on the relative strengths of…

Astrophysics of Galaxies · Physics 2019-08-07 T. J. Davidge

We present the BeppoSAX broad-band X-ray spectrum of the Seyfert 2 galaxy NGC 3281. The source high-energy spectrum is characterized by the nuclear transmitted component, with an absorbing column density of about 2 10^24 cm^-2, while the…

Astrophysics · Physics 2009-11-07 C. Vignali , A. Comastri

We study the composition of the Galactic interstellar medium (ISM) toward the Galactic center region (5 < |l| < 20 degree) by utilizing X-ray absorption features of three bright low-mass X-ray binaries (LMXBs), GX 13+1, GX 5-1, and GX…

Astrophysics · Physics 2009-11-10 Yoshihiro Ueda , Kazuhisa Mitsuda , Hiroshi Murakami , Kyoko Matsushita

We report the first detection of ~10 and ~18 micron silicate dust emissions in a low-luminosity active galactic nucleus (AGN), obtained in Spitzer-IRS 7-37 micron spectroscopy of the Type 1 LINER galaxy NGC3998. Silicate emissions in AGN…

The recent Spitzer detections of the 9.7 micron Si--O silicate emission in type 1 AGNs provide support for the AGN unification scheme. The properties of the silicate dust are of key importance to understanding the physical, chemical and…

Astrophysics · Physics 2009-11-13 M. P. Li , Q. J. Shi , Aigen Li

We report the detection of interstellar silicate dust in the z_abs=0.685 absorber along the sightline toward the gravitationally lensed blazar TXS 0218+357. Using Spitzer Space Telescope Infrared Spectrograph data we detect the 10 micron…

Astrophysics of Galaxies · Physics 2015-06-18 M. C. Aller , V. P. Kulkarni , D. G. York , D. E. Welty , G. Vladilo , N. Liger

Mid-infrared (MIR) spectra observed with Gemini/Michelle were used to study the nuclear region of the Compton-thick Seyfert 2 (Sy 2) galaxy Mrk 3 at a spatial resolution of $\sim$200 pc. No polycyclic aromatic hydrocarbons (PAHs) emission…

Astrophysics of Galaxies · Physics 2014-03-11 Dinalva A. Sales , D. Ruschel-Dutra , M. G. Pastoriza , R. Riffel , Cláudia Winge

We discuss the origin of the ``dusty lukewarm absorber'', which we previously identified in the reddened Seyfert 1 galaxies NGC 3227 and Akn 564. This absorber is characterized by saturated UV absorption lines (C IV, N V) near the systemic…

Astrophysics · Physics 2009-11-07 D. M. Crenshaw , S. B. Kraemer

Results from an analysis of the intrinsic UV absorption in the Seyfert 1 galaxy NGC 3783 are presented. We focus on two new results that demonstrate techniques for deriving important constraints on the physical conditions and geometry of…

Astrophysics · Physics 2007-05-23 Jack R. Gabel , Steven B. Kraemer , D. Michael Crenshaw

Dust plays a central role in the unification theory of active galactic nuclei (AGNs). However, little is known about the nature (e.g., size, composition) of the dust which forms a torus around the AGN. In this Letter we report a systematic…

Astrophysics of Galaxies · Physics 2015-06-22 Jianwei Lyu , Lei Hao , Aigen Li

Using the Spitzer Space Telescope, we have obtained rest frame 9-16mu spectra of 11 quasars and 9 radio galaxies from the 3CRR catalog at redshifts 1.0<z<1.4. This complete flux-limited 178MHz-selected sample is unbiased with respect to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 C. Leipski , M. Haas , S. P. Willner , M. L. N. Ashby , B. J. Wilkes , G. G. Fazio , R. Antonucci , P. Barthel , R. Chini , P. Ogle , R. Siebenmorgen , F. Heymann

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…

Astrophysics · Physics 2009-11-11 A. Poncelet , G. Perrin , H. Sol

We present detailed modeling of the spectral energy distribution (SED) of the spiral galaxies NGC 891, NGC 4013, and NGC 5907 in the far-infrared and submm wavelengths. The model takes into account the emission produced by the diffuse dust…

Astrophysics · Physics 2009-11-10 K. M. Dasyra , E. M. Xilouris , A. Misiriotis , N. D. Kylafis