Results 91 to 100 of about 2,644 (226)

The Distance to the Magellanic Stream: Constraints from Optical Absorption along Stellar Sight Lines

open access: yesThe Astrophysical Journal
The Magellanic Stream is a large tail of neutral and ionized gas originating from tidal and hydrodynamical interactions between the Magellanic Clouds as they orbit the Milky Way (MW).
Sapna Mishra   +4 more
doaj   +1 more source

Physical and Chemical Properties of Galactic Molecular Gas toward QSO J1851+0035

open access: yesThe Astrophysical Journal
Atacama Large Millimeter/submillimeter Array (ALMA) data toward QSO J1851+0035 ( l = 33.°498, b = +0.°194) were used to study absorption lines by Galactic molecular gas.
Kanako Narita   +4 more
doaj   +1 more source

Interstellar X-ray absorption spectroscopy of oxygen, neon, and iron with the CHANDRA LETGS Spectrum of X0614+091

open access: yes, 2001
We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra X-Ray Observatory Low-Energy Transmission Grating Spectrometer (LETGS) spectrum of the low-mass X-ray binary X0614+091.
Kahn, S. M.   +22 more
core   +1 more source

Dust Grain Chemistry in the Diffuse Interstellar Medium toward the Black Hole Transient GX 339–4

open access: yesThe Astrophysical Journal
We present results on X-ray absorption and the dust grain chemistry in the diffuse interstellar medium, based on a new Cycle 25 Chandra High Energy Transmission Grating Spectrometer (HETGS) observational campaign targeting the black hole transient GX 339–
I. Psaradaki   +12 more
doaj   +1 more source

Investigating Silicate, Carbon, and Water in the Diffuse Interstellar Medium: The First Shots from WISCI

open access: yesThe Astrophysical Journal
The dusty interstellar medium (ISM) of the Milky Way is distributed in a complex, cloudy structure. It is fundamental to the radiation balance within the Milky Way, provides a reaction surface to form complex molecules, and is the feedstock for future ...
S. T. Zeegers   +35 more
doaj   +1 more source

Ca II and CH+ interstellar absorption observations in the direction of resolvable binary stars [PDF]

open access: yes, 1997
We report the initial results of a study to probe the small-scale structure in diffuse interstellar clouds by observing optical absorption lines of CH+ at 4232 °A and Ca II K at 3933 °A towards both components in resolvable binary systems.
Palazzi, E., Attolini, M. R., Crane, P.
core  

Ultraviolet Properties of Multiphase Gas toward the Inner Galaxy

open access: yesThe Astrophysical Journal
We present a systematic study of the multiphase interstellar gas in the inner Galaxy using Hubble Space Telescope/STIS absorption spectroscopy of 16 massive stars located at spectroscopic distances between 1.3 and 10 kpc in the region −30° ≲  l  ≲ +30 ...
Frances H. Cashman   +8 more
doaj   +1 more source

Interstellar Absorption and Dust Scattering [PDF]

open access: yes
The study of the interstellar medium (ISM) in the X-rays has entered a golden age with the advent of the X-ray observatories XMM-Newton and Chandra. High-energy resolution allowed to study dust spectroscopic features with unprecedented detail.
Costantini, E.; id_orcid, Corrales, L.
core   +1 more source

The ESO Diffuse Interstellar Band Large Exploration Survey (EDIBLES) [PDF]

open access: yes, 2018
The ESO Diffuse Interstellar Band Large Exploration Survey (EDIBLES) is a Large Programme that is collecting high-signal-to-noise (S/N) spectra with UVES of a large sample of O and B-type stars covering a large spectral range.
Cox, N.L.J.   +48 more
core   +1 more source

Aperture and Resolution Effects on Ultraviolet Star-forming Properties: Insights from Local Galaxies and Implications for High-redshift Observations

open access: yesThe Astrophysical Journal
We present an analysis of the effects of spectral resolution and aperture scale on derived galaxy properties using far-ultraviolet (FUV) spectra of local star-forming galaxies from the International Ultraviolet Explorer ( R ∼ 250, field of view (FOV ...
Ilyse Clark   +4 more
doaj   +1 more source

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