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相关论文: Interstellar Carbon in Translucent Sightlines

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We present interstellar C II (1334.5323 \AA) and C II* (1335.7077 \AA) column density measurements along 14 Galactic sight-lines. These sight-lines sample a variety of Galactic disk environments and include paths that range nearly two…

星系天体物理 · 物理学 2011-02-18 Veena S. Parvathi , Ulysses J. Sofia , Jayant Murthy , B. R. S. Babu

We have reanalyzed the Goddard High Resolution Spectrograph data set presented by Snow et al. which contains the interstellar intersystem C II] 2325A line through the translucent cloud toward HD 24534 (X Persei). In contrast to the results…

天体物理学 · 物理学 2009-10-30 Ulysses J. Sofia , Edward L. Fitzpatrick , David M. Meyer

We present a study of the abundances and physical conditions in the interstellar gas toward the heavily reddened star HD 192639 [E_(B-V) = 0.64], based on analysis of FUSE and HST/STIS spectra covering the range from 912 to 1361 A. This…

天体物理学 · 物理学 2009-11-07 P. Sonnentrucker , S. D. Friedman , D. E. Welty , D. G. York , T. P. Snow

We report on the abundance of interstellar neutral nitrogen (NI) for 30 sightlines, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE) and the Hubble Space Telescope (HST). NI column densities are derived by measuring the…

天体物理学 · 物理学 2008-11-26 Adam G. Jensen , Brian L. Rachford , Theodore P. Snow

We report interstellar FeII and SiII column densities toward six translucent sight lines (A_V >~ 1) observed with the Space Telescope Imaging Spectrograph (STIS). The abundances were determined from the absorption of SiII] at 2335…

天体物理学 · 物理学 2011-02-11 Adam Miller , J. T. Lauroesch , Ulysses J. Sofia , Stefan I. B. Cartledge , David M. Meyer

We discuss the interstellar absorption from many atomic and molecular species seen in high-resolution $HST$/STIS UV and high-S/N optical spectra of the moderately reddened B3-5~V star HD~62542. This remarkable sight line exhibits both very…

星系天体物理 · 物理学 2020-07-08 Daniel E. Welty , Paule Sonnentrucker , Theodore P. Snow , Donald G. York

We use new Space Telescope Imaging Spectrograph (STIS) and archival Goddard High Resolution Spectrograph (GHRS) observations to study interstellar B II 1362 and O I 1355 absorption along seven sightlines. Our new column density…

天体物理学 · 物理学 2009-10-31 J. Christopher Howk , Kenneth R. Sembach , Blair D. Savage

We present a comprehensive examination of interstellar P and Cl abundances based on an analysis of archival spectra acquired with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope and the Far Ultraviolet Spectroscopic…

星系天体物理 · 物理学 2023-05-30 Adam M. Ritchey , J. M. Brown , S. R. Federman , Paule Sonnentrucker

We have used archival far-ultraviolet spectra from observations made by HST/STIS and FUSE to determine the column densities and rotational excitation temperatures for CO and H2, respectively, along the lines of sight to 23 Galactic O and B…

天体物理学 · 物理学 2009-01-19 Eric B. Burgh , Kevin France , Stephan R. McCandliss

We present column density measurements of the HD molecule in the interstellar gas toward 17 Galactic stars. The values for the seven most heavily reddened sightlines, with E(B-V) = 0.38-0.72, are derived from observations with the Far…

天体物理学 · 物理学 2008-11-26 S. Lacour , M. K. Andre , P. Sonnentrucker , F. Le Petit , D. E. Welty , J. -M. Desert , R. Ferlet , E. Roueff , D. G. York

The nature of the Local Interstellar Cloud (LIC) is highly constrained by the combination of in situ heliospheric and line-of-sight data towards nearby stars. We present a new interpretation of the LIC components of the absorption line data…

天体物理学 · 物理学 2011-02-11 Jonathan D. Slavin , Priscilla C. Frisch

We report the first ensemble results from the FUSE survey of molecular hydrogen in lines of sight with A_V $\gtrsim$ 1 mag. We have developed techniques for fitting computed profiles to the low-J lines of H2, and thus determining column…

We present an analysis of high resolution HST Space Telescope Imaging Spectrograph (STIS) observations of O I 1356 and H I Lyman-alpha absorption in 36 sight lines that probe a variety of Galactic disk environments and include paths that…

天体物理学 · 物理学 2009-11-10 Stefan I. B. Cartledge , J. T. Lauroesch , David M. Meyer , Ulysses J. Sofia

We present a comprehensive survey of boron abundances in diffuse interstellar clouds from observations made with the Space Telescope Imaging Spectrograph (STIS) of the Hubble Space Telescope. Our sample of 56 Galactic sight lines is the…

星系天体物理 · 物理学 2011-02-02 A. M. Ritchey , S. R. Federman , Y. Sheffer , D. L. Lambert

The H II region W40 harbors a small group of young, hot stars behind roughly 9 magnitudes of visual extinction. We have detected gaseous carbon monoxide (CO) and diatomic carbon (C_2) in absorption toward the star W40 IRS 1a. The 2-0 R0,…

天体物理学 · 物理学 2009-10-31 R. Y. Shuping , T. P. Snow , R. Crutcher , B. L. Lutz

Using archival, high-resolution far-ultraviolet HST/STIS spectra of 34 Galactic O and B stars, we measure CI column densities and compare them with measurements from the literature of CO and H_2 with regard to understanding the presence of…

星系天体物理 · 物理学 2014-11-20 Eric B. Burgh , Kevin France , Edward B. Jenkins

We present new measurements of the interstellar gas-phase oxygen abundance along the sight lines towards 19 early-type galactic stars at an average distance of 2.6 kpc. We derive O {\small I} column densities from {\it HST}/STIS…

We present measurements of the 3.4-micron hydrocarbon dust absorption feature, and four visual diffuse interstellar bands, for twelve highly reddened (9.0<A(V)<15.8), early-type stars identified from the Stephenson (1992) catalogue,…

天体物理学 · 物理学 2009-11-07 M. G. Rawlings , A. J. Adamson , D. C. B. Whittet

We have obtained high resolution (FWHM = 4.4 km/s) Keck spectra of images A and C of the gravitationally lensed QSO Q1422+231. The images are separated by 1.3" on the sky. In an absorption system at z = 3.538 gas column density variations…

天体物理学 · 物理学 2007-05-23 Michael Rauch , Wallace L. W. Sargent , Thomas A. Barlow

We present the analysis of a sub-DLA system (log N(H^0)=20.0+/-0.15, z_abs=2.69) toward SDSS J123714+064759 (z_em=2.78). Using the VLT/UVES and X-shooter spectrographs, we detect H2, HD and CO molecules in absorption with log…

宇宙学与河外天体物理 · 物理学 2015-05-19 P. Noterdaeme , P. Petitjean , C. Ledoux , S. Lopez , R. Srianand , S. D. Vergani
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