Interstellar extinction from photometric surveys: application to four high-latitude areas [PDF]
Information on interstellar extinction and dust properties may be obtained from modern large photometric surveys data. Virtual Observatory facilities allow users to make a fast and correct cross-identification of objects from various surveys. It yields a
Malkov Oleg +13 more
doaj +5 more sources
Fitting procedure for estimating interstellar extinction at high galactic latitudes
We determine the interstellar extinction in the selected high-latitude areas of the sky based on Gaia EDR3 astrometry and photometry and spectroscopic data from RAVE survey.
Oleg Yu. Malkov, Dana Kovaleva
exaly +2 more sources
Interstellar extinction and interstellar polarization: Old and new models [PDF]
The review contains an analysis of the observed and model curves of the interstellar extinction and polarization. The observations mainly give information on dust in diffuse and translucent interstellar clouds.
N V Voshchinnikov
exaly +2 more sources
LAMOST Spectroscopy and Gaia Photo-Astrometry for an Interstellar Extinction Study
The aim of this work is to establish the present accuracy and convergence of available estimates of galactic extinction. We determine the galactic interstellar extinction in selected high-latitude areas of the sky based on Gaia DR3 astrometry and ...
Oleg Yu. Malkov +2 more
exaly +3 more sources
Interstellar Extinction and Elemental Abundances: Individual Sight Lines [PDF]
While it is well recognized that both the Galactic interstellar extinction curves and the gas-phase abundances of dust-forming elements exhibit considerable variations from one sight line to another, as yet most of the dust extinction modeling efforts ...
Wenbo Zuo, Ai-Gen Li, Gang Zhao
semanticscholar +1 more source
The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium [PDF]
We present a new model of interstellar dust in which large grains are a single composite material, “astrodust,” and nanoparticle-sized grains come in distinct varieties including polycyclic aromatic hydrocarbons (PAHs). We argue that a single-composition
B. Hensley, B. Draine
semanticscholar +1 more source
Measuring Optical Extinction toward Young Stellar Objects Using Diffuse Interstellar Bands [PDF]
Line-of-sight extinction estimates of well-studied young T Tauri and Herbig Ae/Be stars are based on many different measurements and analysis methods. This has resulted in wide scatter among the published A V values for the same star.
A. Carvalho, L. Hillenbrand
semanticscholar +1 more source
Detection of PAH Absorption and Determination of the Mid-infrared Diffuse Interstellar Extinction Curve from the Sight Line toward Cyg OB2-12 [PDF]
The sight line toward the luminous blue hypergiant Cyg OB2-12 is widely used to study interstellar dust on account of its large extinction (AV ≃ 10 mag) and the fact that this extinction appears to be dominated by dust typical of the diffuse interstellar
B. Hensley, B. Draine
semanticscholar +1 more source
An Analysis of the Shapes of Interstellar Extinction Curves. VIII. The Optical Extinction Structure [PDF]
New Hubble Space Telescope/STIS optical spectra were obtained for a sample of early-type stars with existing International Ultraviolet Explorer UV spectra. These data were used to construct optical extinction curves whose general properties are discussed
D. Massa, E. Fitzpatrick, K. Gordon
semanticscholar +1 more source
Interstellar Extinction and Elemental Abundances [PDF]
Elements in the interstellar medium (ISM) exist in the form of gas or dust. The interstellar extinction and elemental abundances provide crucial constraints on the composition, size, and quantity of interstellar dust.
Wenbo Zuo, Ai-Gen Li, Gang Zhao
semanticscholar +1 more source

