English
Related papers

Related papers: A rapid occultation event in NGC 3227

200 papers

We obtained optical spectra of the counterpart of the ultraluminous X-ray source NGC 5408 X-1 using the FORS spectrograph on the VLT. The spectra show strong high excitation emission lines, He{\sc ii} $\lambda$4686 and [Ne{\sc V}]…

High Energy Astrophysical Phenomena · Physics 2010-01-15 Philip Kaaret , Stephane Corbel

We present the analysis of XMM-Newton and Swift optical-UV and X-ray observations of the Seyfert-1/QSO Mrk 509, part of an unprecedented multi-wavelength campaign, investigating the nuclear environment of this AGN. The XMM-Newton data are…

We present results from several years of fast optical photometry of 4U0614+091 (V1055 Orionis), a candidate ultracompact X-ray binary most likely consisting of a neutron star and a degenerate secondary. We find evidence for strong…

Solar and Stellar Astrophysics · Physics 2015-05-28 Pasi Hakala , Phil Charles , Panu Muhli

As part of our multiwavelength campaign of GX 339-4 observations in 1996 we present the rapid X-ray variability observed July 26 using the RXTE when the source was in a hard state (= soft X-ray low state). We found that the source was…

Astrophysics · Physics 2009-10-31 I. A. Smith , E. P. Liang

Long X-ray observations of bright Active Galactic Nuclei show that X-ray eclipses, with durations from a few hours to a few days, are rather common. This opens up a new window of opportunity in the search for signatures of relativistic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 G. Risaliti , E. Nardini , M. Elvis , L. Brenneman , M. Salvati

We report on a quasi-periodic variation at $\sim1$ Hz during a fast X-ray outburst of a high-mass X-ray binary MAXI J0709$-$159 / LY CMa observed by the Neutron-star interior composition explorer (NICER). The new X-ray transient MAXI…

The reflection nebula NGC 2023 was observed by a rocket-borne long-slit imaging spectrograph in the 900 -- 1400 Angstrom bandpass on 2000 February 11. A spectrum of the star, as well as that of the nebular scattered light, was recorded.…

Astrophysics · Physics 2009-11-07 Eric B. Burgh , Stephan R. McCandliss , Paul D. Feldman

We analyze the X-ray properties for a sample of 23 high probability AGN candidates with ultraviolet variability identified in Wasleske et al. (2022). Using data from the Chandra X-ray Observatory and the XMM-Newton Observatory, we find…

Astrophysics of Galaxies · Physics 2024-05-31 Erik J. Wasleske , Vivienne F. Baldassare

We have discovered an ultrasoft X-ray transient source, 2XMMi J184725.1-631724, which was detected serendipitously in two XMM-Newton observations in the direction of the center of the galaxy IC 4765-f01-1504 at a redshift of 0.0353. These…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Dacheng Lin , Eleazar R. Carrasco , Dirk Grupe , Natalie A. Webb , Didier Barret , Sean A. Farrell

We present serendipitous simultaneous radio and X-ray light curves of the dwarf Seyfert galaxy UGC 6728 spanning 5 years. The X-ray light curve exhibits a flaring period, followed by a gradual rise and decline. Throughout these events, the…

Astrophysics of Galaxies · Physics 2026-01-23 Krista Lynne Smith , Macon Magno , Michael Koss

We select a sample of nearby Ultraluminous X-ray sources with long XMM-Newton observations and analyse all the available XMM-Newton data using both X-ray spectral fitting techniques and hardness-intensity diagrams. The sample includes IC…

High Energy Astrophysical Phenomena · Physics 2014-03-05 Fabio Pintore , Luca Zampieri , Anna Wolter , Tomaso Belloni

We report on the RXTE detection of a sudden increase in the absorption column density, $N_\mathrm{H}$, during the 2011 May outburst of GX 304-1. The $N_\mathrm{H}$ increased up to ${\sim}16\times 10^{22}$ atoms cm$^{-2}$, which is a factor…

When emission in a conical relativistic jet ceases abruptly (or decays sharply), the observed decay light curve is controlled by the high-latitude "curvature effect". Recently, Uhm & Zhang found that the decay slopes of three GRB X-ray…

High Energy Astrophysical Phenomena · Physics 2016-08-03 Lan-Wei Jia , Z. Lucas Uhm , Bing Zhang

We present a thorough study of the Changing-Look Active Galactic Nucleus (CL-AGN) Mrk 1018, utilizing an extensive dataset spanning optical, UV, and X-ray spectro-photometric data from 2005 to 2019. We analysed X-ray spectra and broad-band…

High Energy Astrophysical Phenomena · Physics 2023-12-14 S. Veronese , C. Vignali , P. Severgnini , G. A. Matzeu , M. Cignoni

We test the "reprocessing paradigm" of the optical -- UV AGN variability by detailed modeling of the correlated X-ray -- optical (3590 and 5510 Angstrem) variability of the recent multiwavelength campaign of NGC 3516. We produce model…

Astrophysics · Physics 2009-10-31 Demos Kazanas , Sergei Nayakshin

We present a complete analysis of the hard X-ray (2-10 keV) properties of the Seyfert galaxy NGC 1365, based on a 60 ks XMM-Newton observation performed in January 2004. The two main results are: 1) We detect an obscuring cloud with…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 G. Risaliti , G. Miniutti , G. Fabbiano , M. Salvati , A. Baldi , V. Braito , S. Bianchi , G. Matt , J. Reeves , R. Soria , A. Zezas

We report on the detection of a statistically significant flare-like event in the Mg~II~$\lambda$ 2798~\AA\ emission line and the UV~Fe~II band of CTA~102 during the outburst of autumn 2017. The ratio between the maximum and minimum of…

High Energy Astrophysical Phenomena · Physics 2020-03-11 Vahram Chavushyan , Víctor M. Patiño-Álvarez , Raúl A. Amaya-Almazán , Luis Carrasco
‹ Prev 1 8 9 10 Next ›