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Related papers: Digging process in NGC 6951: the molecular disc bu…

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We present a Chandra ACIS-S observation of the nuclear region of the nearby spiral galaxy M51 (NGC 5194), which has a low-luminosity Seyfert 2 nucleus. The X-ray image shows the nucleus, southern extranuclear cloud, and northern loop, the…

Astrophysics · Physics 2009-11-06 Yuichi Terashima , Andrew S. Wilson

We present new results for the molecular gas, dust emission and the ionized gas in J1023+1952, an HI rich intergalactic star-forming tidal dwarf galaxy candidate. It is located at the projected intersection of two faint stellar tidal…

Astrophysics · Physics 2009-11-13 U. Lisenfeld , C. G. Mundell , E. Schinnerer , P. N. Appleton , J. Allsopp

We map the optical and near-infrared (NIR) emission-line flux distributions and kinematics of the inner 320$\times$535pc$^2$ of the elliptical galaxy NGC1052. The integral field spectra were obtained with the Gemini Telescope using the…

We have mapped the 2.6 mm CO (1-0) emission in three optically selected "Toomre Sequence" mergers (NGC 520, NGC 3921, NGC 4676). The molecular gas distribution is well resolved by the observations. For NGC 520 and NGC 4676A, the nuclear gas…

Astrophysics · Physics 2007-05-23 Min S. Yun , J. E. Hibbard

We present the largest sample to date of giant molecular clouds (GMCs) in a substantial spiral galaxy other than the Milky Way. We map the distribution of molecular gas with high resolution and image fidelity within the central 5 kpc of the…

Deep, narrow-band \Ha\ and 6584 \AA\ [\Nii ] CCD images of the peculiar, infrared excess B[e] star MWC~922 reveal a collimated, bipolar jet orthogonal to the previously detected extended nebula. The jet consists of a pair of $\sim$0.15 pc…

Astrophysics of Galaxies · Physics 2019-02-06 John Bally , Zen H. Chia

We present a deep XMM-Newton observation of the extremely massive, rapidly rotating, relativistic-jet-launching spiral galaxy 2MASX J23453268-0449256. Diffuse X-ray emission from the hot gaseous halo around the galaxy is robustly detected…

Astrophysics of Galaxies · Physics 2020-11-11 M. S. Mirakhor , S. A. Walker , J. Bagchi , A. C. Fabian , A. J. Barth , F. Combes , P. Dabhade , L. C. Ho , M. B. Pandge

NGC 1052 offers the possibility to study the obscuring torus around a supermassive black hole, predicted by the standard model of active galactic nuclei, over a wide range of wavelengths from the radio to the X-ray regime. We present a…

Astrophysics · Physics 2009-11-10 M. Kadler , E. Ros , A. P. Lobanov , H Falcke , J. A. Zensus

We present high-resolution (~ 4") 12CO (J = 1 - 0) mapping observations with high - velocity resolution (~ 2.6 km s^{-1}) toward the disk of flocculent galaxy NGC 5055, using the Nobeyama Millimeter Array in order to study the physical…

Astrophysics · Physics 2015-06-24 Tomoka Tosaki , Yasuhiro Shioya , Nario Kuno , Kouichiro Nakanishi , Takashi Hasegawa

We present new Hubble, Gemini-S, and Chandra observations of the radio galaxy 0313-192, which hosts a 350-kpc double source and jets, even though previous data have suggested that it is a spiral galaxy. We measure the bulge scale and…

Astrophysics · Physics 2009-11-11 William C. Keel , Raymond E. White , Frazer N. Owen , Michael J. Ledlow

We have used the IRAM Plateau de Bure Interferometer and the Expanded Very Large Array to obtain a high resolution map of the CO(6-5) and CO(1-0) emission in the lensed, star-forming galaxy SMMJ2135-0102 at z=2.32. The kinematics of the gas…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Mark Swinbank , Padelis Papadopoulos , Pierre Cox , Melanie Krips , Rob Ivison , Ian Smail , Alasdair Thomson , Roberto Neri , Johan Richard , Harald Ebeling

We present observational results of water vapor maser emission with our high-sensitivity 22 GHz VLBI imaging of the Seyfert galaxy NGC 1068. In this galaxy, there are the following four nuclear radio sources; NE, C, S1, and S2. Among them,…

Astrophysics of Galaxies · Physics 2022-12-14 Yuna Morishima , Hiroshi Sudou , Aya Yamauchi , Yoshiaki Taniguchi , Naomasa Nakai

In the massive star-forming region IRAS 21078+5211, a highly fragmented cluster (0.1~pc in size) of molecular cores is observed, located at the density peak of an elongated (1~pc in size) molecular cloud. A small (1~km/s per 0.1~pc) LSR…

We present a study of the outflowing ionized gas in the resolved narrow-line region (NLR) of the Seyfert 2 galaxy Mrk 573, and its interaction with an in- ner dust/gas disk, based on Hubble Space Telescope (HST) WFPC2 and STIS observations.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 T. C. Fischer , D. M. Crenshaw , S. B. Kraemer , H. R. Schmitt , M. L. Trippe

We present spectroscopic observations of the stellar motions in the disk of the superthin edge-on spiral galaxy IC 5249 and re-analyse synthesis observations of the HI. We find that the HI rotation curve rises initially to about 90-100…

Astrophysics · Physics 2009-11-07 P. C. van der Kruit , J. Jimenez-Vicente , M. Kregel , K. C. Freeman

Double-lobed radio sources associated with active galactic nuclei (DRAGNs) are typically found in elliptical galaxies, while supermassive black holes (SMBHs) in disk galaxies rarely produce powerful kpc-scale jets. However, the growing…

Astrophysics of Galaxies · Physics 2025-08-08 Seung Yeon Lee , Jae-Young Kim

We present a spatially resolved analysis of ionized gas at the nuclear region of the nearby galaxy NGC 1068. While NGC 1068 has been known to have gas outflows driven by its active galactic nucleus (AGN), more complex kinematical signatures…

Astrophysics of Galaxies · Physics 2021-02-24 Jaejin Shin , Jong-Hak Woo , Minjin Kim , Junfeng Wang

We present observations of the HCN and HCO+ J=1-0 transitions in the center of the nearby spiral galaxy NGC 6946 made with the BIMA and CARMA interferometers. Using the BIMA SONG CO map, we investigate the change in the I_HCN/I_CO and I_…

Astrophysics · Physics 2009-11-13 E. S. Levine , Tamara T. Helfer , R. Meijerink , Leo Blitz

We investigated the jet width profile with distance along the jet in the nearby radio galaxy NGC 1052 at radial distances between $\sim300$ to $4 \times 10^7$ Schwarzschild Radii($R_{\rm S}$) from the central engine on both their…

The detailed distribution and kinematics of the atomic and the CO-bright molecular hydrogen in the disc of the Milky Way inside the Solar circle are derived under the assumptions of axisymmetry and pure circular motions. We divide the…

Astrophysics of Galaxies · Physics 2017-11-22 A. Marasco , F. Fraternali , J. M. van der Hulst , T. Oosterloo
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