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Related papers: X-ray Absorption Line Spectroscopy of the Galactic…

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We report on strong H2 and CO absorption from gas within the host galaxy of gamma-ray burst (GRB) 080607. Analysis of our Keck/LRIS afterglow spectrum reveals a very large HI column density (NHI = 10^22.70 cm^-2) and strong metal-line…

The intrinsic X-ray emission of Gamma-Ray Bursts (GRBs) is often found to be absorbed over and above the column density through our own galaxy. The extra component is usually assumed to be due to absorbing gas lying within the host galaxy…

High Energy Astrophysical Phenomena · Physics 2015-06-15 R. L. C. Starling , R. Willingale , N. R. Tanvir , A. E. Scott , K. Wiersema , P. T. O'Brien , A. J. Levan , G. C. Stewart

Hot, \logT\ $\sim$ 7.5, gas was recently discovered in the Milky Way in extragalactic sightlines. In order to determine its location, here we present sightlines to Galactic X-ray binaries (XRBs) passing through the Interstellar Medium…

Astrophysics of Galaxies · Physics 2024-07-25 Armando Lara-DI , Yair Krongold , Smita Mathur , Manami Roy , Rebecca L. McClain , Sanskriti Das , Anjali Gupta

The Chandra AO1 HETGS observation of the micro-quasar GRS 1915+105 in the low hard state reveals (1) neutral K absorption edges from Fe, Si, Mg, and S in cold gas, and (2) highly ionized (Fe XXV and Fe XXVI) absorption attributed to a hot…

Astrophysics · Physics 2009-09-17 J. C. Lee , C. S. Reynolds , R. Remillard , N. S. Schulz , E. G. Blackman , A. C. Fabian

We present a theory for interpreting the sodium lines detected in transmission spectra of exoplanetary atmospheres. Previous analyses employed the isothermal approximation and dealt only with the transit radius. By recognising the…

Earth and Planetary Astrophysics · Physics 2015-06-24 Kevin Heng , Aurélien Wyttenbach , Baptiste Lavie , David K. Sing , David Ehrenreich , Christophe Lovis

We have made HI 21cm-line absorption measurements using the GMRT towards 15 directions in the Galaxy which are known to have high random velocity clouds as seen in the optical absorption lines of CaII and NaI. For the first time, in 6 out…

Astrophysics · Physics 2007-05-23 Rekhesh Mohan , K. S. Dwarakanath , G. Srinivasan , Jayaram N. Chengalur

Nitrogen is one of the most abundant metals in the interstellar medium (ISM), and thus it constitutes an excellent test to study a variety of astrophysical environments, ranging from nova to active galactic nuclei. We present a detailed…

High Energy Astrophysical Phenomena · Physics 2021-05-12 Efrain Gatuzz , Javier A. García , Timothy R. Kallman

To detect a warm-hot intergalactic medium associated with the large-scale structure of the universe, we observed a quasar behind the Virgo cluster with XMM-Newton. With a net exposure time of 54 ks, we marginally detected an OVIII K alpha…

This paper presents an analysis of XMM X--ray spectra of the quasar 1ES 1553+113, in search for absorption lines from the intervening warm--hot intergalactic medium. A search for OVII, OVIII and NeIX resonance absorption lines was performed…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-14 D. Spence , M. Bonamente , J. Nevalainen , T. Tuominen , J. Ahoranta , J. de Plaa , W. Liu , N. Wijers

Many of the baryons associated with a galaxy reside in its circumgalactic medium (CGM), in a diffuse volume-filling phase at roughly the virial temperature. Much of the oxygen produced over cosmic time by the galaxy's stars also ends up…

Astrophysics of Galaxies · Physics 2019-08-14 G. M. Voit

We discuss the detectability of Warm/Hot Intergalactic medium (WHIM) via the absorption lines toward bright point sources with a future X-ray satellite mission, XEUS. While we consider bright QSOs as specific examples, the methodology can…

We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Transmission Grating Spectrometer spectrum of the low mass X-ray binary X0614+091. We measure the column densities in O and Ne, and find direct…

We use FUSE and STIS spectra to study intergalactic absorption towards the quasar PG1259+593 (z=0.478). We identify 135 intergalactic absorption lines with equivalent widths >10mA, tracing 78 absorption components in 72 Ly alpha/beta…

Astrophysics · Physics 2009-11-10 Philipp Richter , Blair D. Savage , Todd M. Tripp , Kenneth R. Sembach

We detect seven distinct absorbing systems in the high-resolution X-ray spectrum of the Seyfert 1 galaxy IC 4329A, taken with XMM-Newton. Firstly we detect absorption due to cold gas in our own Galaxy and warm gas in the Galactic halo or…

We present the first localized detections of the cold neutral medium (CNM) in IC10, offering a rare view of dense atomic gas in a low-metallicity (0.27 solar metallicity) dwarf galaxy. As a low-metallicity starburst, IC10's interstellar…

We have used STIS aboard HST to search for Lyman-alpha (Lya) absorption in the outer regions of nine nearby (cz<6000 km/s) galaxies using background QSOs and AGN as probes. The foreground galaxies are intercepted between 26 and 199 h-1 kpc…

Astrophysics · Physics 2017-08-23 David V. Bowen , Max Pettini , J. Chris Blades

We present early science results from the First Large Absorption Survey in HI (FLASH), a spectroscopically blind survey for 21-cm absorption lines in cold hydrogen HI gas at cosmological distances using the Australian Square Kilometre Array…

We present new observations on PKS 2155-304 with the Chandra Low Energy Transmission Grating Spectrometer (LETG), using the Advanced CCD Imaging Spectrometer (ACIS). We confirm the detection of an absorption line plausibly identified as…

Astrophysics · Physics 2009-11-13 Taotao Fang , Claude R. Canizares , Yangsen Yao

We study the X-ray properties of LINER sources with definite detection of a broad H(alpha) emission line in their optical spectra, LINER 1s from Ho et al. sample. These objects preferentially harbor a low luminosity active nucleus at the…

Astrophysics of Galaxies · Physics 2015-05-28 G. Younes , D. Porquet , B. Sabra , J. N. Reeves

We use the EAGLE (Evolution and Assembly of GaLaxies and their Environments) cosmological simulation to study the distribution of baryons, and far-ultraviolet (O VI), extreme-ultraviolet (Ne VIII) and X-ray (O VII, O VIII, Ne IX, and Fe…

Astrophysics of Galaxies · Physics 2020-09-07 Nastasha A. Wijers , Joop Schaye , Benjamin D. Oppenheimer