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相关论文: GMRT Observations of NGC 3079

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We present results from multi-frequency polarization-sensitive Very Large Array observations of the Seyfert-starburst composite galaxy NGC3079. Our sensitive radio observations reveal a plethora of radio filaments comprising the radio lobes…

星系天体物理 · 物理学 2019-10-09 Biny Sebastian , Preeti Kharb , C. P. O Dea , E. J. M. Colbert , S. A. Baum

Using the Effelsberg radio telescope at 4.85GHz and 8.35 GHz we discovered large symmetric lobes of polarized radio emission around the strongly HI deficient Virgo cluster spiral galaxy NGC4569. These lobes extend up to 24 kpc from the…

天体物理学 · 物理学 2007-05-23 K. T. Chyzy , M. Soida , D. J. Bomans , Ch. Balkowski , R. Beck , M. Urbanik

Very deep neutral hydrogen (HI) observations of the edge-on spiral galaxy NGC 3079 with the Westerbork Synthesis Radio Telescope (WSRT) are presented. The galaxy has been studied extensively in different wavelengths and known for its…

宇宙学与河外天体物理 · 物理学 2009-08-28 N. Shafi , R. Morganti , T. Oosterloo , R. Booth

We present high-resolution, high-sensitivity radio continuum observations of the nearby spiral galaxy NGC 2997 at 332, 616 and 1272 MHz using the Giant Metrewave Radio Telescope (GMRT). The integrated spectrum of this galaxy has a spectral…

星系天体物理 · 物理学 2015-05-28 J. Kodilkar , N. G. Kantharia , S. Ananthakrishnan

We present deep neutral hydrogen (HI) observations of the starburst/Seyfert galaxy NGC 3079 and its environment, obtained with the Westerbork Synthesis Radio Telescope. Our observations reveal previously unknown components, both in HI…

星系天体物理 · 物理学 2015-10-14 N. Shafi , T. A. Oosterloo , R. Morganti , S. Colafrancesco , R. Booth

within 24 lines with 80 characters) We present ^12CO (1-0) observations in the central 4.5 kpc (1 arcmin) of the Halpha/Radio lobe galaxy NGC 3079 with the Nobeyama Millimeter Array. The molecular gas shows four components: a main disk,…

天体物理学 · 物理学 2009-11-07 J. Koda , Y. Sofue , K. Kohno , H. Nakanishi , S. Onodera , S. K. Okumura , Judith A. Irwin

We present sensitive, high-resolution radio observations of the circumnuclear region of the barred spiral galaxy NGC6951. These observations reveal a ring of radio emission with many discrete components and a marginally resolved nuclear…

天体物理学 · 物理学 2009-11-07 D. J. Saikia , B. Phookun , A. Pedlar , K. Kohno

We report the results of the spatial and spectral analysis of the ROSAT HRI and PSPC observations of the edge-on spiral galaxy NGC 3079. We detected several sources in the field of NGC 3079 with both PSPC and HRI, and complex emission from…

天体物理学 · 物理学 2007-05-23 W. Pietsch , G. Trinchieri , A. Vogler

We have performed high-resolution synthesis observations of the 12CO (J=1-0) line emission from the radio lobe edge-on spiral NGC 3079 using a 7-element mm-wave interferometer at Nobeyama, which consisted of the 45-m telescope and 6-element…

天体物理学 · 物理学 2009-10-31 Y. Sofue , J. Koda , K. Kohno , S. K. Okumura , M. Honma , A. Kawamura , Judith A. Irwin

We present low frequency observations at $315$ and $745$ MHz from the upgraded Giant Metrewave Radio Telescope (uGMRT) of the edge-on, nearby galaxy NGC $4631$. We compare the observed surface brightness profiles along the minor axis of the…

星系天体物理 · 物理学 2022-02-09 Aditi Vijayan , K. S. Dwarakanath , Biman B. Nath , Ruta Kale

Starburst galaxies are undergoing intense episodes of star formation. In these galaxies, gas is ejected into the surrounding environment through winds created by the effect of hot stars and supernova explosions. When interacting with the…

星系天体物理 · 物理学 2024-03-12 C. A. Galante , J. Saponara , G. E. Romero , P. Benaglia

The upgraded Giant Metrewave Radio Telescope (GMRT) has been used to map the cluster A2065 at z = 0.0726. We report the discovery of a remnant radio galaxy at the peripheral cluster region. The spatially resolved radio emission from the…

星系天体物理 · 物理学 2021-07-06 Dharam V. Lal

We present multi-frequency, radio-continuum and HI observations of NGC4438, the highly-disturbed, active galaxy in the Virgo cluster, with the VLA and the GMRT. High-resolution observations with the VLA at 4860 and 8460 MHz show the…

天体物理学 · 物理学 2009-11-13 Ananda Hota , D. J. Saikia , Judith A. Irwin

We report the discovery of a `Triple-Double Radio Galaxy (TDRG)' J1216+0709 detected in deep low-frequency Giant Metrewave Radio Telescope (GMRT) observations. J1216+0709 is only the third radio galaxy, after B0925+420 and Speca, with three…

星系天体物理 · 物理学 2016-08-03 Veeresh Singh , C. H. Ishwara-Chandra , Preeti Kharb , Shweta Srivastava , P. Janardhan

We report on C-band (5 - 7 GHz) observations of the galaxy, NGC~2992, from the CHANG-ES sample. This galaxy displays an embedded nuclear double-lobed radio morphology within its spiral disk, as revealed in linearly polarized emission but…

Radio observations can show how cluster galaxies are affected by various environmental factors. We made three frequency radio-polarimetric VLA observations and performed sensitive XMM-Newton observations in X-rays and UV light of NGC4254.…

天体物理学 · 物理学 2009-11-13 K. T. Chyzy , M. Ehle , R. Beck

We present new continuum VLA observations of the nearby Sy 1.5 galaxy NGC 5033, made at 4.9 and 8.4 GHz on 8 April 2003. Combined with VLA archival observations at 1.4 and 4.9 GHz made on 7 August 1993, 29 August 1999, and 31 October 1999,…

天体物理学 · 物理学 2019-08-19 Miguel A. Perez-Torres , Antonio Alberdi

The Seyfert 2 galaxy NGC3079 is one of the nearest radio-weak AGN. We have carried out multi-frequency, multi-epoch VLBI observations of this object and detected new components, proper motion of the order of 0.1 c, strong spectral…

天体物理学 · 物理学 2007-05-23 E. Middelberg , T. P. Krichbaum , A. L. Roy , A. Witzel , J. A. Zensus

Sensitive images of low-level, Mpc-sized radio cocoons offer new opportunities to probe large scale intergalactic gas flows outside clusters of galaxies. New radio images of high surface brightness sensitivity at strategically chosen…

We present new, high frequency radio observations of the merging galaxy clusters PLCK G287.0+32.9, Abell 2744, and Bullet. These clusters are known to host $\sim$Mpc scale sources, known as radio halos, which are formed by the acceleration…

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