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相关论文: VLA detection of OH absorption from the elliptical…

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We used the Plateau de Bure Interferometer to observe $\lambda$3mm J=1-0 absorption lines of \hcop, HCN and CO toward the core of the nearby elliptical, megamaser-host galaxy NGC1052. The lines are relatively weak, with peak optical depths…

天体物理学 · 物理学 2009-11-10 H. Liszt , R. Lucas

The bright radio structure of the LINER elliptical galaxy NGC1052 is dominated by bi-symmetric jets on parsec scales. Features move outward on both sides of the core at v_{app}~0.26c. We have established the occurrence of free-free…

天体物理学 · 物理学 2007-05-23 R. C. Vermeulen , E. Ros , J. A. Zensus , K. I. Kellermann , M. H. Cohen , H. J. van Langevelde

We present multi-frequency simultaneous VLBA observations at 15, 22 and 43 GHz towards the nucleus of the nearby radio galaxy NGC 1052. These three continuum images reveal a double-sided jet structure, whose relative intensity ratios imply…

宇宙学与河外天体物理 · 物理学 2010-11-02 S. Sawada-Satoh , S. Kameno , K. Nakamura , D. Namikawa , K. M. Shibata , M. Inoue

We present Giant Metrewave Radio Telescope (GMRT) observations of OH absorption in B3~1504+377 ($z \sim 0.673$) and PKS 1413+135 ($z \sim 0.247$). OH has now been detected in absorption towards four intermediate redshift systems, viz. the…

天体物理学 · 物理学 2009-11-07 Nissim Kanekar , Jayaram N Chengalur

We examine the 0.1 to 10.0 keV X-ray spectrum of the bright nuclear LINER galaxy NGC 1052, one of two elliptical galaxies known to contain a luminous H2O maser. The observed 2.0-10.0 keV spectrum is unusually flat (photon index Gamma~0.2)…

天体物理学 · 物理学 2009-10-31 K. A. Weaver , A. S. Wilson , C. Henkel , J. A. Braatz

We present multi-frequency simultaneous VLBA observations at 15, 22 and 43 GHz towards the nucleus of the nearby radio galaxy NGC 1052. These three continuum images reveal a double-sided jet structure, whose relative intensity ratios imply…

We present deep GMRT OH and WSRT HI absorption spectra of the $z = 0.6846$ gravitational lens toward B0218+357. Both the 1665 MHz and 1667 MHz OH lines are clearly detected for the first time while a new wide absorption component was…

天体物理学 · 物理学 2009-11-10 N. Kanekar , J. N. Chengalur , A. G. de Bruyn , D. Narasimha

We present the first VLBI detection of HCN molecular absorption in the nearby active galactic nucleus NGC 1052. Utilizing the 1 milliarcsecond resolution achieved by the Korean VLBI Network, we have spatially resolved the HCN absorption…

We report the detection of the satellite 18 cm OH lines at 1612 and 1720 MHz in the z=0.2467 molecular absorption system toward the radio source PKS 1413+135. The two OH lines are conjugate; the 1612 MHz line is seen in absorption while the…

天体物理学 · 物理学 2009-11-10 Jeremy Darling

We investigate the correlation between OH and H2 column densities in diffuse Galactic clouds, in order to identify potential molecular tracers of interstellar H2. For this, we analyse near-UV spectra extracted from the ESO/VLT archives…

星系天体物理 · 物理学 2023-06-09 Katherine Rawlins , Bhaswati Mookerjea

Broad hydroxyl (OH) absorption-lines in the 1667 MHz and 1665 MHz transition towards the central region of NGC 3079 have been observed at high resolution with the European VLBI Network (EVN). Velocity fields of two OH absorption components…

天体物理学 · 物理学 2009-11-10 Y. Hagiwara , H. -R. Kloeckner , W. Baan

We study the structure and kinematics of the OH-streamer and the +80 km/s cloud and their interactions with the circumnuclear disk (CND) and with other molecular clouds in the vicinity of the Galactic centre (GC), and we map OH absorption…

星系天体物理 · 物理学 2015-11-04 Roland Karlsson , Aage Sandqvist , Kambiz Fathi , Sergio Martín

We present 92cm observations of the high-redshift galaxy B2 0902+343 (z=3.40) with the Westerbork Synthesis Radio Telescope (WSRT). Twenty-one cm HI is detected in absorption, at a depth of 15.9 mJy (=~6\sigma) and rest frame velocity width…

天体物理学 · 物理学 2009-11-07 Ann Marie Cody , Robert Braun

In the circumnuclear region of the nearby radio galaxy NGC~1052. Our $\lambda$3mm VLBI observations with the Korean VLBI Network have spatially resolved the broad HCO$^{+}$ absorption at a velocity range of 1350--1850 km~s$^{-1}$ against a…

This is a paper on young jet material in a frustratingly complex environment. NGC 1052 has a compact, flat- or GHz-peaked-spectrum radio nucleus consisting of bi-symmetric jets, oriented close to the plane of the sky. Many features on both…

天体物理学 · 物理学 2009-11-07 R. C. Vermeulen , E. Ros , K. I. Kellermann , M. H. Cohen , J. A. Zensus , H. J. van Langevelde

(Abridged) We discuss multiple VLBI continuum and spectral line observations and WSRT spectroscopy of NGC 1052. Sub-parsec scale features move outward at approximately 0.26c in bi-symmetric jets, most likely oriented near the plane of the…

天体物理学 · 物理学 2009-11-07 R. C. Vermeulen , E. Ros , K. I. Kellermann , M. H. Cohen , J. A. Zensus , H. J. van Langevelde

We present Giant Meterwave Radio Telescope (GMRT) observations of the HI 21 cm line and Very Large Array (VLA) observations of the OH 18 cm line from the Seyfert 2 galaxy Mrk 1. HI emission is detected from both Mrk 1 and its companion NGC…

天体物理学 · 物理学 2009-11-07 A. Omar , K. S. Dwarakanath , M. Rupen , K. R. Anantharamaiah

We present results from VLBA observations of the 1667 and 1665 MHz OH lines in the two OH megamaser galaxies IRAS12032+1707 and IRAS14070+0525. For IRAS12032+1707 we also present Arecibo HI absorption data. Almost all OH emission previously…

天体物理学 · 物理学 2009-11-10 Y. M. Pihlstrom , W. A. Baan , J. Darling , H. -R. Klockner

OH absorption against PSR B1718-35 at (l,b) =351.688,+0.671 has been discovered at 1665 and 1667 MHz using the Green Bank Telescope. The absorption appears to arise at the interface of an HII region and a molecular cloud which are likely…

天体物理学 · 物理学 2009-11-13 Anthony H. Minter
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