Results 81 to 90 of about 5,560 (224)
O VI in the local interstellar medium
International audienceWe report preliminary results of a search for O VI absorption in the spectra of ∼100 hot DA white dwarfs observed by the FUSE satellite.
Forbes, AE +11 more
core +1 more source
Measuring the properties of the cold neutral medium (CNM) in low-metallicity galaxies provides insights into heating and cooling mechanisms in early Universe-like environments.
Nickolas M. Pingel +17 more
doaj +1 more source
We present a model for interstellar extinction dust, in which we assume a bimodal distribution of extinction carriers, a dispersion of core-mantle grains, supplemented by a collection of PAHs in free molecular form.
C. Cecchi-Pestellini +7 more
doaj +1 more source
A survey of ultraviolet interstellar absorption lines
A telescope-spectrometer on the Copernicus spacecraft made possible the measurement of many ultraviolet absorption lines produced by the interstellar gas. The present survey provides data on ultraviolet absorption lines in the spectra of 88 early-type stars.
R. C. Bohlin +6 more
openaire +1 more source
H i Kinematics and the E(B − V)/N(H i) Ratio
The λ 21 cm H i emission that is used to trace the gas-to-dust ratio at high Galactic latitudes has contributions from material beyond the Milky Way disk, with uncertain and likely subsolar metallicity and dust content.
Harvey Liszt
doaj +1 more source
Absorption and scattering by interstellar dust in the silicon K-edge of GX 5-1
We study the absorption and scattering of X-ray radiation by interstellar dust particles, which allows us to access the physical and chemical properties of dust.
Zeegers, S. T. +23 more
core +1 more source
Understanding variations in the dust extinction curve is imperative for using dust as a tracer of local structure in the interstellar medium, understanding dust chemistry, and performing extinction corrections.
Andrew K. Saydjari, Gregory M. Green
doaj +1 more source
Interstellar absorption lines toward Cep OB4
An analysis of optical echelle spectra towards nine stars in the Cep OB4 association is presented. Interstellar absorption lines which arise in the (1, 0) and (2, 0) bands of the CN A $^2\Pi$ – X $^2\Sigma^+$ red system towards BD+66° 1661, BD+66 ...
R. Gredel
core +1 more source
Interstellar NaI and CaII absorption observed towards the Cygnus Loop SNR
We present high resolution spectra ($R \sim 5$ km s-1) of the interstellar NaI and CaII absorption lines observed towards 9 early-type stars with distances ranging from 250 to 2300 pc in the line-of-sight towards the Cygnus Loop Supernova Remnant (SNR).
S. Sallmen +3 more
core +1 more source
TWO PHOTON ABSORPTION BY MOLECULAR HYDROGEN AS A MECH ANISM FOR INTERSTELLAR EXTINCTION
Author Institution: Electro-Optical SystemsA review is given of the theory of two-photon absorption with emphasis on selection rules, orders-of-magnitude of cross-sections and the concept of a ``two-photon absorption spectrum.
Duardo, J. A.
core

