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相关论文: Neutral hydrogen gas within and around NGC 1316

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We present and interpret observations of atomic and molecular gas toward the southern elliptical galaxy NGC 1316 (Fornax A), a strong double-lobe radio source with a disturbed optical morphology that includes numerous shells and loops. The…

天体物理学 · 物理学 2009-11-06 C. Horellou , J. H. Black , J. H. van Gorkom , F. Combes , J. M. van der Hulst , V. Charmandaris

The MeerKAT Fornax Survey maps the distribution and kinematics of atomic neutral hydrogen gas (HI) in the nearby Fornax galaxy cluster using the MeerKAT telescope. The 12 deg^2 survey footprint covers the central region of the cluster out…

We present multi-wavelength imagery of the merger remnant galaxy NGC 1316 with an objective to study the content of dust and its association with the other phases of the ISM. Color-index maps as well as extinction maps derived for this…

宇宙学与河外天体物理 · 物理学 2018-08-08 S. P. Deshmukh , B. T. Tate , N. D. Vagshette , S. K. Pandey , M. K. Patil

We present MeerKAT Fornax Survey HI observations of NGC 1427A, a blue irregular galaxy with a stellar mass of 2e+9 Msun located near the centre of the Fornax galaxy cluster. Thanks to the excellent resolution (1 to 6 kpc spatially, 1.4 km/s…

The MeerKAT Fornax Survey is conducting a thorough examinationof the nearby Fornax galaxy cluster to understand how galaxies lose their cold gas and stop forming stars in low-mass clusters (M$_{\rm vir} \leq 10^{14}$ M$_\odot$). We are…

星系天体物理 · 物理学 2025-07-25 F. M. Maccagni , P. Serra

We present MeerKAT neutral hydrogen (HI) observations of the Fornax A group, that is likely falling into the Fornax cluster for the first time. Our HI image is sensitive to 1.4 x 10$^{19}$ cm$^{-2}$ over 44.1 km s$^{-1}$, where we detect HI…

We present VLA observations of the neutral hydrogen and radio continuum of NGC 34 (= NGC 17 = Mrk 938). This object is an ideal candidate to study the fate of gas in mergers, since, as shown by an optical study done by Schweizer & Seitzer…

宇宙学与河外天体物理 · 物理学 2015-05-20 Ximena Fernandez , J. H. van Gorkom , Francois Schweizer , Joshua E. Barnes

The HI structure and kinematics of the peculiar starburst galaxy NGC 3310 (Arp 217, UGC 5786) are discussed. New evidence bearing on the origin of the starburst is presented. The bulk of HI coincides with the bright optical disk and shows…

天体物理学 · 物理学 2009-11-06 M. Kregel , R. Sancisi

We report on multi-object spectroscopy of 37 candidate star clusters around the giant early-type radio galaxy NGC 1316 (Fornax A), the brightest galaxy in the Fornax cluster. For the star clusters in this sample, we measure a mean radial…

天体物理学 · 物理学 2009-10-31 Paul Goudfrooij , Jennifer Mack , Markus Kissler-Patig , Georges Meylan , Dante Minniti

We present Australia Telescope Compact Array (ATCA) HI imaging of the edge-on galaxy NGC 1596, which was recently found to have counter-rotating ionized gas in its center (<15"). We find a large HI envelope associated with a nearby…

天体物理学 · 物理学 2009-11-11 Aeree Chung , Baerbel Koribalski , Martin Bureau , J. H. van Gorkom

We present new MeerKAT 21cm spectral line observations of the neutral hydrogen gas in the compact galaxy group Stephan's Quintet (HCG 92). These data provide a significantly improved view of the atomic gas distribution and kinematics in the…

We present new HI observations from the Australia Telescope Compact Array and deep optical imaging from OmegaCam on the VLT Survey Telescope of NGC 1427A, an arrow-shaped dwarf irregular galaxy located in the Fornax cluster. The data reveal…

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

The merger remnant NGC 1316 (Fornax A) is one of the most important objects regarding the investigation of merger-related processes. We use kinematical data of globular clusters (GCs) and the diffuse stellar light to investigate the global…

星系天体物理 · 物理学 2014-09-17 Tom Richtler , Michael Hilker , Brijesh Kumar , Lilia P. Bassino , Matias Gomez , Boris Dirsch

The light of the merger remnant NGC 1316 is dominated by old and intermediate-age stars. The only sign of current star formation in this big galaxy is the HII region SH2, an isolated star cluster complex with a ring-like morphology and an…

星系天体物理 · 物理学 2017-05-24 T. Richtler , B. Husemann , M. Hilker , T. H. Puzia , F. Bresolin , M. Gómez

We report on high-sensitivity neutral hydrogen observations toward the gas-rich interacting galaxies NGC 3395/3396 with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Compared to previous observations carried out by the…

星系天体物理 · 物理学 2024-08-01 Nai-Ping Yu , Ming Zhu , Jin-Long Xu , Chuan-Peng Zhang , Hai-Yang Yu , Xiao-Lan Liu , Peng Jiang , Mei Ai

The early-type galaxy NGC 1316 hosts about 10^7 solar masses of dust within a central radius of 5 kpc. These prominent dust structures are believed to have an external origin, which is also a popular interpretation for other dusty…

星系天体物理 · 物理学 2020-11-11 T. Richtler , M. Hilker , E. Iodice

(abridged) Here we present HI line and 20-cm radio continuum data of the nearby galaxy pair NGC1512/1510 as obtained with the Australia Telescope Compact Array. These are complemented by GALEX UV-, SINGG Halpha- and Spitzer mid-infrared…

宇宙学与河外天体物理 · 物理学 2015-05-14 Baerbel S. Koribalski , Angel R. Lopez-Sanchez

We present HI line and 20-cm radio continuum observations of the NGC 1511 galaxy group obtained with the Australia Telescope Compact Array. The data reveal an extended, rather disturbed HI distribution for the peculiar starburst galaxy NGC…

天体物理学 · 物理学 2009-11-10 B. Koribalski , E. Manthey

We have observed NGC 1316 (Fornax A) with the ROSAT HRI. In this paper, we present the results of these observations and we complement them with the spectral analysis of the archival PSPC data. The spectral properties suggest the presence…

天体物理学 · 物理学 2009-10-30 Dong-Woo Kim , Giuseppina Fabbiano , Glen Mackie
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