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相关论文: NGC 4869 in the Coma cluster: twist, wrap, overlap…

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Observations of the radio remnant of Supernova 1987A using the Australia Telescope Compact Array in the 12-mm band on 2003 July 31 (day 6002.7 after the explosion) give the first fully resolved radio image of the supernova remnant. The…

天体物理学 · 物理学 2009-11-11 R. N. Manchester , B. M. Gaensler , L. Staveley-Smith , M. J. Kesteven , A. K. Tzioumis

We present the first multi-frequency analysis of the candidate ultra-steep spectrum radio halo in the galaxy cluster PLCKESZ G171.94$-$40.65, using the upgraded Giant Metrewave Radio telescope (uGMRT; 400 MHz), and Karl G. Jansky Very Large…

We present an analysis of the Fe K line profile of NGC 4151 by using long ASCA observation data obtained in May 1995. The unprecedented good data quality, which is much better in the energy band around 6.4 keV than that of the famous…

天体物理学 · 物理学 2009-10-31 Junxian. Wang , Youyuan. Zhou , Tinggui. Wang

The optical line and continuum emission in the very high ionization Galactic planetary nebula (PN) NGC 4361 (PN G294.1 +43.6), has been mapped with VLT MUSE Wide Field normal mode (4750-9300A) commissioning observations. The PN is larger…

太阳与恒星天体物理 · 物理学 2024-10-16 J. R. Walsh , A. Monreal Ibero , J. Laging , M. Romeijnders

We present new 1.5-8.5 GHz Very Long Baseline Array (VLBA) observations and 0.32-1.26 GHz Giant Meterwave Radio Telescope (GMRT) observations of J0354-1340, which is the only known radio-quiet (RQ) or radio-intermediate (RI) narrow-line…

We present evidence for a broad, ionized Fe K line in the XMM-Newton spectrum of the broad-line radio galaxy (BLRG) 4C+74.26. This is the first indication that the innermost regions of the accretion flow in BLRGs contain thin, radiatively…

天体物理学 · 物理学 2009-11-10 D. R. Ballantyne , A. C. Fabian

We report results from the simultaneous XRISM (183 ks) and NuSTAR (62 ks) observations of the Seyfert-2 galaxy NGC 4388. This AGN has the brightest Fe K$\alpha$ line among Compton-thin, obscured sources. To model the reflection continuum…

We present the results of new Suzaku observations of the Coma Cluster, the X-ray brightest, nearby, merging system hosting a well studied, typical giant radio halo. It has been previously shown that, on the western side of the cluster, the…

高能天体物理现象 · 物理学 2016-01-20 Y. Uchida , A. Simionescu , T. Takahashi , N. Werner , Y. Ichinohe , S. W. Allen , O. Urban , K. Matsushita

We have mapped the total sky brightness at 1465 MHz in two adjacent 60-degree declination bands with the portable 5.5-m parabolic reflector of the Galactic Emission Mapping (GEM) project, an on-going international collaboration to survey…

天体物理学 · 物理学 2007-05-23 C. Tello , T. Villela , G. F. Smoot , S. Torres , M. Bersanelli

We report on large-scale, regular morphological patterns found in the radio jet of the nearby radio galaxy NGC 6251. Investigating morphological properties of this radio jet from the nucleus to a radial distance of $\sim$ 300 arcsec…

天体物理学 · 物理学 2009-10-31 H. Sudou , Y. Taniguchi

The analysis of a deep (579 ks) Chandra ACIS pointing of the elliptical galaxy NGC4278, which hosts a low luminosity AGN and compact radio emission, allowed us to detect extended emission from hot gas out to a radius of \sim 5 kpc, with a…

高能天体物理现象 · 物理学 2015-06-05 S. Pellegrini , J. Wang , G. Fabbiano , D. W. Kim , N. J. Brassington , J. S. Gallagher , G. Trinchieri , A. Zezas

We have undertaken a study of the globular cluster (GC) systems of a large sample of elliptical and spiral galaxies in order to test predictions of galaxy formation models. Here we present results for the giant Virgo elliptical NGC 4472…

天体物理学 · 物理学 2009-10-31 K. L. Rhode , S. E. Zepf

We present the results of observations of the radio halo in the Coma galaxy cluster at 4.8 GHz performed with the Sardinia Radio Telescope. The radio halo in this cluster is detected for the first time at this frequency with a statistical…

宇宙学与河外天体物理 · 物理学 2026-03-20 P. Marchegiani , M. Murgia , F. Loi , V. Vacca , F. Govoni , S. Cocchi , F. Gandossi

Giant double-lobed radio source 4C34.47 displays a straight one-sided jet, measuring a record length of 380kpc, in its double-lobed radio structure. Assuming an intrinsically symmetric two-sided jet structure the radio source jet axis must…

星系天体物理 · 物理学 2015-05-19 S. Hocuk , P. D. Barthel

We present results from a 49.4 ks Chandra/ACIS-S observation of the nearby ($z$=0.059) X-shaped FRII radio galaxy 3C~403. This is the first Chandra observation of an X-shaped radio galaxy, and one of the goals of this pioneering study is to…

天体物理学 · 物理学 2009-11-10 R. P. Kraft , M. J. Hardcastle , D. M. Worrall , S. S. Murray

We present radio maps of the head-tail radio galaxy, 3C 129 at 240 and 610 MHz using the Giant Metrewave Radio Telescope. We have studied in detail the morphology of the source and the distribution of spectral index over the object. We find…

天体物理学 · 物理学 2015-06-24 Dharam Vir Lal , A. Pramesh Rao

We present the kpc-scale behaviour of the powerful extragalactic radio source Hercules A and the behaviour of the intracluster gas in which the radio source is situated. We have found that Hercules A exhibits a strong Laing-Garrington…

天体物理学 · 物理学 2009-11-07 Nectaria A. B. Gizani , M. A. Garrett , J. P. Leahy

We present X-ray spectroscopic and morphological analyses using Chandra ACIS and ROSAT observations of the giant elliptical galaxy NGC 4472 in the Virgo cluster. We discuss previously unobserved X-ray structures within the extended galactic…

天体物理学 · 物理学 2009-11-10 B. A. Biller , C. Jones , W. R. Forman , R. Kraft , T. Ensslin

We study the exponential scale length of total radio emission, the spectral index distribution, and the linear radio polarization in the Scd galaxy M33. Observations were carried out using the 3.6 cm dual channel and the 6.2 cm four channel…

天体物理学 · 物理学 2009-11-13 F. S. Tabatabaei , M. Krause , R. Beck

We have mapped the head-tail radio galaxy, 3C 129 at 240 and 610 MHz using the GMRT and studied the detailed morphology and spectral index variations in this object. This is the first attempt to observe a sample of head-tail sources at low…

天体物理学 · 物理学 2007-05-23 Dharam Vir Lal , A. Pramesh Rao