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相关论文: VLT observations of Compact Central Objects

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We report the serendipitous discovery of VVV-WIT-12, an unusual variable source that seems to induce variability in its surrounding nebula. The source belongs to the rare objects that we call WITs (short for What Is This?) discovered within…

We present a radio/optical study of a sample of BL Lac objects at arcsecond and milliarcsecond resolution. The sample consists of 30 nearby (z<0.2) BL Lacs, mostly X-ray selected. These nearby objects are weak in the radio, yet we have…

天体物理学 · 物理学 2007-05-23 M. Giroletti , G. Giovannini , G. B. Taylor , R. Falomo

Compact Symmetric Objects (CSOs), young jetted-AGN of overall projected size <1 kpc, are of great interest due to their youth and evolution. The classification was introduced to distinguish between ~95% of powerful compact extragalactic…

Vela Jr. is one of the youngest and likely nearest among the known galactic supernova remnants (SNRs). Discovered in 1997 it has been studied since then at quite a few wavelengths, that spread over almost 20 decades in energy. Here we…

天体物理学 · 物理学 2007-05-23 A. F. Iyudin , B. Aschenbach , V. Burwitz , K. Dennerl , M. Freyberg , F. Haberl , M. Filipovic

We have selected a sample of 80 candidates for obscured radio-loud active galactic nuclei and presented their basic optical/near-infrared (NIR) properties in Paper 1. In this paper, we present both high-resolution radio continuum images for…

星系天体物理 · 物理学 2016-03-16 Ting Yan , John T. Stocke , Jeremy Darling , Emmanuel Momjian , Soniya Sharma , Nissim Kanekar

We present the second in a series of results in which we have searched for undiscovered neutron stars in supernova remnants (SNRs). This paper deals with the largest six SNRs in our sample, too large for Chandra or XMM-Newton to cover in a…

天体物理学 · 物理学 2009-11-11 D. L. Kaplan , B. M. Gaensler , S. R. Kulkarni , P. O. Slane

Compact symmetric objects (CSOs) trace the earliest phases of radio-galaxy growth; however, robust classification is difficult when radio cores are weak or invisible. We aim to develop and test a Gaia+VLBI approach that utilizes the…

星系天体物理 · 物理学 2026-01-14 T. An , Y. Zhang , S. Frey , W. A. Baan , A. Wang

A Chandra X-ray observation has detected an unresolved source at the center of the supernova remnant Kes 79. The best single-model fit to the source spectrum is a blackbody with an X-ray luminosity Lx (0.3-8.0 keV) = 7 x 10^{33} ergs…

天体物理学 · 物理学 2009-11-07 F. D. Seward , P. O. Slane , R. K. Smith , M. Sun

A Chandra image of the central X-ray source RX J0007.0+7303 in the supernova remnant CTA 1 reveals a point source, a compact nebula, and a bent jet, all of which are characteristic of energetic, rotation-powered pulsars. Using the MDM 2.4m…

天体物理学 · 物理学 2009-11-10 J. P. Halpern , E. V. Gotthelf , F. Camilo , D. J. Helfand , S. M. Ransom

We report the results of our search for the near infrared counterpart of the microquasar 1E 1740.7-2942 using the VLT (Based on observations collected at the European Southern Observatory, Chile (ESO No 63.H-0261)). For the first time,…

天体物理学 · 物理学 2007-05-23 Josep Marti , I. Felix Mirabel , Sylvain Chaty , Luis F. Rodriguez

We have carried out a study of the neutral hydrogen in the direction of the X-ray source 1E 161348-5055, a compact central object (CCO) located in the interior of the supernova remnant (SNR) RCW 103. The HI 21 cm line observations were…

天体物理学 · 物理学 2009-11-10 E. M. Reynoso , A. J. Green , S. Johnston , W. M. Goss , G. M. Dubner , E. B. Giacani

G15.9+0.2 is a Galactic shell-type supernova remnant (SNR), which was detected in radio and has been confirmed in X-rays based on Chandra observations. An X-ray point source CXOUJ181852.0-150213 has been detected and suggested to be an…

高能天体物理现象 · 物理学 2018-07-11 Manami Sasaki , Minja M. Maäkelaä , Dmitry Klochkov , Andrea Santangelo , Valery Suleimanov

Central compact objects (CCOs) constitute a population of radio-quiet, slowly-spinning ($\ge$100 ms) young neutron stars with anomalously high thermal X-ray luminosities. Their spin-down properties imply weak dipole magnetic fields…

高能天体物理现象 · 物理学 2015-06-22 Slavko Bogdanov , C. -Y. Ng , Victoria M. Kaspi

The Catalina Real Time Survey (CRTS) has found over 500 cataclysmic variable (CV) candidates, most of which were previously unknown. We report here on followup spectroscopy of 36 of the brighter objects. Nearly all the spectra are typical…

太阳与恒星天体物理 · 物理学 2015-06-05 John R. Thorstensen , Julie N. Skinner

Context. Central compact objects (CCOs) are a peculiar class of neutron stars, primarily encountered close to the center of young supernova remnants (SNRs) and characterized by thermal X-ray emission. Aims. Our goal is to perform a…

高能天体物理现象 · 物理学 2021-07-14 Martin G. F. Mayer , Werner Becker

We present results of EVN observations of eleven GHz-Peaked-Spectrum (GPS) radio sources at 2.3/8.4 GHz. These sources are from the classical ''bright'' GPS source samples with peak flux densities $>$ 0.2 Jy and spectral indices $\alpha <…

天体物理学 · 物理学 2007-05-23 L. Xiang , D. Dallacasa , P. Cassaro , D. Jiang , C. Reynolds

We present early results from the first IR imaging of the weak X-ray sources discovered in a recent Chandra survey towards the Galactic Centre. From our VLT observations we will identify likely counterparts to a sample of the hardest…

A new sample of candidate Compact Steep Spectrum (CSS) sources that are much weaker than the CSS source prototypes has been selected from the VLA FIRST catalogue. MERLIN `snapshot' observations of the sources at 5 GHz indicate that six of…

天体物理学 · 物理学 2009-11-11 Magdalena Kunert-Bajraszewska , Andrzej Marecki , Peter Thomasson , Ralph E. Spencer

Despite about a decade of observations, very little is known about the optical and infrared (IR) emission properties of the Soft Gamma-ray Repeaters (SGRs) and of the Anomalous X-ray Pulsars (AXPs), the magnetar candidates, and about the…

高能天体物理现象 · 物理学 2009-11-13 R. P. Mignani , N. Rea , V. Testa , G. L. Israel , G. Marconi , S. Mereghetti , P. Jonker , R. Turolla , R. Perna , S. Zane , G. Lo Curto , S. Chaty

We present the results of EVN polarization observations of fourteen GHz-Peaked-Spectrum (GPS) radio sources at 5 GHz. These sources were selected from bright GPS source samples and we aimed at finding Compact Symmetric Objects (CSOs). We…

天体物理学 · 物理学 2016-08-30 Liu Xiang , Cormac Reynolds , Richard Strom , Daniele Dallacasa