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相关论文: An atomic hydrogen bridge fueling NGC 4418 with ga…

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VV 655, a dwarf irregular galaxy with HI tidal debris, is a companion to the lenticular luminous infrared galaxy (LIRG) NGC 4418. NGC 4418 stands out among nearby LIRGs due to its dense central concentration of molecular gas and the dusty,…

The aim of this study is to constrain the dynamics, structure and feeding of the compact nucleous of NGC4418, and to reveal the nature of the main hidden power source: starburst or AGN. We obtained high spatial resolution observations of…

星系天体物理 · 物理学 2015-06-16 F. Costagliola , S. Aalto , K. Sakamoto , S. Martín , R. Beswick , S. Muller , H. -R. Klöckner

We present high spatial resolution 21 cm HI maps of the interacting galaxy pair NGC 7714/7715. We detect a massive (2 x 10**9 M(sun)) HI bridge connecting the galaxies that is parallel to but offset from the stellar bridge. A chain of HII…

天体物理学 · 物理学 2009-10-30 Beverly J. Smith , Curt Struck , Richard W. Pogge

High resolution, Hubble Space Telescope (HST) near-infrared and Keck mid-infrared images of the heavily extinguished, infrared luminous galaxy NGC 4418 are presented. These data make it possible to observe the imbedded near-infrared…

We present near-infrared and millimeter investigations of the nucleus of the infrared luminous galaxy NGC 4418, which previous observations suggest possesses a powerful buried AGN. We found the following main results: (1) The infrared…

天体物理学 · 物理学 2009-11-10 Masatoshi Imanishi , Kouichiro Nakanishi , Nario Kuno , Kotaro Kohno

We have observed the nucleus of the nearby luminous infrared galaxy NGC 4418 with subarcsec resolution at 860 and 450 micron for the first time to characterize its hidden power source. A ~20 pc (0.1") hot dusty core was found inside a 100…

宇宙学与河外天体物理 · 物理学 2015-06-12 Kazushi Sakamoto , Susanne Aalto , Francesco Costagliola , Sergio Martin , Youichi Ohyama , Martina C. Wiedner , David J. Wilner

The galaxy NGC 4418 contains one of the most compact obscured nuclei within a luminous infrared galaxy (LIRG) in the nearby Universe. This nucleus contains a rich molecular gas environment and an unusually high ratio of infrared to radio…

星系天体物理 · 物理学 2014-06-04 E. Varenius , J. E. Conway , I. Martí-Vidal , S. Aalto , R. Beswick , F. Costagliola , H. -R. Klöckner

We present new radio continuum, 21 cm HI, and 2.6 mm CO data for the peculiar radio galaxy NGC 4410A and its companion NGC 4410B, and compare with available optical and X-ray maps. Our radio continuum maps show an asymmetric…

天体物理学 · 物理学 2009-10-31 Beverly J. Smith

The radio source 4C12.50 has often been suggested to be a prime candidate for the link between ultraluminous infrared galaxies and young radio galaxies. A VLBI study of the neutral hydrogen in the nuclear regions of this object shows that…

We investigated the inner buried nucleus of a nearby luminous infrared galaxy NGC 4418 using high-resolution spectroscopy of fundamental carbon monoxide (CO) ro-vibrational absorptions around $4.67 \mu$m for the first time. This method…

How a seemingly `dead' host galaxy provides fuel for its active galactic nuclei (AGN) remains an unresolved problem. Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we present a new high-sensitivity atomic-hydrogen…

星系天体物理 · 物理学 2025-12-19 Jin-Long Xu , Nai-Ping Yu , Ming Zhu , Chuan-Peng Zhang , Xiao-Lan Liu , Mei Ai , Peng Jiang

Herschel/PACS spectroscopy of the luminous infrared galaxies NGC4418 and Arp220 reveals high excitation in H2O, OH, HCN, and NH3. In NGC4418, absorption lines were detected with E_low>800 K (H2O), 600 K (OH), 1075 K (HCN), and 600 K (NH3),…

Spatial and kinematical correlations between HI and CO (2-1) emission of the southern spiral galaxy NGC4945 are studied with a common angular (23 arcsec) and velocity resolution (7 km/s). The 21cm continuum emission is also observed. The HI…

天体物理学 · 物理学 2009-11-07 M. Ott , J. B. Whiteoak , C. Henkel , R. Wielebinski

Observations of the neutral atomic hydrogen (HI) in the nuclear starburst galaxy NGC 4945 with MeerKAT are presented. We find a large amount of halo gas, previously missed by HI observations, accounting for 6.8% of the total HI mass. This…

We report the detection of absorption features in the 6-8 micron region superimposed on a featureless mid-infrared continuum in NGC 4418. For several of these features this is the first detection in an external galaxy. We compare the…

天体物理学 · 物理学 2009-10-31 H. W. W. Spoon , J. V. Keane , A. G. G. M. Tielens , D. Lutz , A. F. M. Moorwood

We present WSRT, VLA and VLBI observations of the HI absorption in the radio galaxy NGC 315. The main result is that two HI absorbing systems are detected against the central region. In addition to the known highly redshifted, very narrow…

宇宙学与河外天体物理 · 物理学 2015-05-14 R. Morganti , A. B. Peck , T. A. Oosterloo , G. van Moorsel , A. Capetti , R. Fanti , P. Parma , H. R. de Ruiter

We present Australia Compact Telescope Array (ATCA) 21-cm observations of the nearby low-excitation radio galaxy (LERG) NGC 3100. This is the brightest galaxy of a loose group and hosts a young ($\sim 2$ Myr) radio source. The ATCA…

星系天体物理 · 物理学 2023-07-05 F. M. Maccagni , I. Ruffa , A. Loni , I. Prandoni , R. Ragusa , D. Kleiner , P. Serra , E. Iodice , M. Spavone

We present new atomic hydrogen (HI) observations of the collisional ring galaxy NGC 922 obtained using the Australia Telescope Compact Array. Our observations reveal for the first time the vast extent of the HI disc of this galaxy. The HI…

Using long-slit optical spectra obtained with the 2-m telescope at IUCAA Girawali Observatory, we show that the radio source J094221.98+062335.2 (z=0.123) is associated with a galaxy pair undergoing a major merger. Its companion is a normal…

星系天体物理 · 物理学 2015-08-06 R. Srianand , N. Gupta , E. Momjian , M. Vivek

We investigate the molecular gas properties of the deeply obscured luminous infrared galaxy NGC 4418. We address the excitation of the complex molecule HC3N to determine whether its unusually luminous emission is related to the nature of…

宇宙学与河外天体物理 · 物理学 2015-05-18 F. Costagliola , S. Aalto
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