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相关论文: The Cartwheel ring under X-ray light

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The existence of a massive black hole in the center of the Milky Way, coinciding with the radio source Sgr A*, is being established on more and more solid ground. In principle, this black hole, acting as a gravitational lens, is able to…

天体物理学 · 物理学 2011-02-11 Valerio Bozza , Luigi Mancini

An enigmatic, small class of IR and X-ray luminous sources, named ``Composite'' starburst/Seyfert galaxies, has been defined from IRAS and RASS data. The objects have optical spectra dominated by the features of HII galaxies (plus, in some…

The excellent quality of the Chandra observation of NGC 5846 reveals a complex X-ray morphology of the central regions of this galaxy. An intriguing morphological similarity between the X-ray and the optical line emission, discovered before…

天体物理学 · 物理学 2009-11-07 Ginevra Trinchieri , Paul Goudfrooij

We present a 10-year X-ray light curve and the spectra of a peculiar X-ray transient in the spiral galaxy M81. The source was below the detection limit of ROSAT PSPC before 1993, but it brightened substantially in 1993, with luminosities…

天体物理学 · 物理学 2009-11-07 Kajal Ghosh , Douglas Swartz , Allyn Tennant , Kinwah Wu

We present the first observation of planet-induced stellar X-ray activity, identified for the HD 179949 system, using Chandra / ACIS-S. The HD 179949 system consists of a close-in giant planet orbiting an F9V star. Previous ground-based…

天体物理学 · 物理学 2009-11-13 S. H. Saar , M. Cuntz , V. L. Kashyap , J. C. Hall

Deep Hubble Space Telescope images of superlative resolution obtained for the distant rich cluster AC114 (z=0.31) reveal a variety of gravitational lensing phenomena for which ground-based spectroscopy is available. We present a luminous…

天体物理学 · 物理学 2009-10-22 Ian Smail , Warrick J. Couch , Richard S. Ellis , Ray M. Sharples

Our 5 ks Chandra ACIS-S observation of the globular cluster NGC 6652 detected 7 X-ray sources, 3 of which are previously unidentified. This cluster hosts a well-known bright low-mass X-ray binary, source A (or XB 1832-330). Source B shows…

高能天体物理现象 · 物理学 2015-05-28 G. Coomber , C. O. Heinke , H. N. Cohn , P. M. Lugger , J. E. Grindlay

Transferring a significant fraction of the magnetic flux from a dense cloud core is essential in the star formation process. A ring-like structure produced by magnetic flux loss has been predicted theoretically, but no observational…

(abridged)We present the observations of the pair of interacting galaxies NGC6285/86 carried out with the 6m SAO RAS telescope by using 1D and 2D spectroscopy. The observations of NGC6286 with a long-slit spectrograph (UAGS) near the…

天体物理学 · 物理学 2009-11-10 L. V. Shalyapina , A. V. Moiseev , V. A. Yakovleva , V. A. Hagen-Thorn , A. N. Burenkov

We consider strong gravitational lensing by nearby stars. Using our wave-optical treatment of lensing phenomena, we study Einstein rings that may form around nearby stellar lenses. It is remarkable that these rings are bright and large…

天体物理仪器与方法 · 物理学 2023-02-13 Slava G. Turyshev , Viktor T. Toth

Sub-arcsecond resolution Chandra observations of Eta Carinae reveal a 40 arcsec X 70 arcsec ring or partial shell of X-ray emission surrounding an unresolved, bright, central source. The spectrum of the central source is strongly absorbed…

天体物理学 · 物理学 2009-11-06 F. D. Seward , Y. M. Butt , M. Karovska , A. Prestwich. E. M. Schlegel , M. Corcoran

An objective prism H alpha survey has shown that there is a population of early type spiral galaxies in nearby clusters with strong central bursts of star formation which could be due to galaxy--galaxy tidal interactions. Such galaxies are…

天体物理学 · 物理学 2007-05-23 C. Moss , M. Whittle , J. E. Pesce , H. Navarro

We report the detection of a gravitationally lensed galaxy by the nearby spiral galaxy CGCG 012-070 ($z = 0.048$) using Integral Field Unit (IFU) observations with the Near-Infrared Spectrograph (NIRSpec) instrument on board the James Webb…

We analyse all the available Chandra observations of the Cartwheel Galaxy and its compact group, taken between 2001 and 2008, with the main aim of addressing the variability in the X-ray band for this spectacular collisional ring galaxy. We…

高能天体物理现象 · 物理学 2023-04-05 Chiara Salvaggio , Anna Wolter , Andrea Belfiore , Monica Colpi

High-mass X-ray binary systems are powered by the stellar wind of their donor stars. The X-ray state of Cygnus X-1 is correlated with the properties of the wind which defines the environment of mass accretion. Chandra-HETGS observations…

We present images of the peculiar galaxy Arp~10 which reveal two rings of concurrent star formation. Apart from a bright ring visible on early photographs of the system, an even brighter inner ring of \ion{H}{2} regions is found within the…

天体物理学 · 物理学 2014-10-13 V. Charmandaris , P. N. Appleton , A. P. Marston

We report the discovery of a unique object in the MeerKAT Galaxy Cluster Legacy Survey (MGCLS) using the machine learning anomaly detection framework Astronomaly. This strange, ring-like source is 30' from the MGCLS field centred on Abell…

星系天体物理 · 物理学 2023-02-09 Michelle Lochner , Lawrence Rudnick , Ian Heywood , Kenda Knowles , Stanislav S. Shabala

This paper presents new Chandra and BeppoSAX observations aimed at investigating the optical/X-ray mismatch in the enigmatic class of the Composite galaxies, discovered by a cross-correlation of IRAS and ROSAT all sky survey catalogues.…

NGC 1232 is a face-on spiral galaxy and a great laboratory for the study of star-formation due to its proximity. We obtained high spatial resolution H{\alpha} images of this galaxy, with adaptive optics, using the SAM instrument at the SOAR…

We report the serendipitous discovery of an "Einstein Ring" in the optical band from the Sloan Digital Sky Survey (SDSS) data and associated four images of a background source. The lens galaxy appears to be a nearby dwarf spheroid at a…

天体物理学 · 物理学 2011-02-11 Kajal K Ghosh , D. Narasimha