Add to ORKGOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the PacificHD 62542 is situated in a line of sight toward a ridge of dark matter in the Gum Nebula. That region is under the influence of UV radiation and stellar winds from hot stars. We use for the first time interstellar polarization and extinction data from the ultraviolet to the infrared in order to study and quantify the influence of such an environment on the size of the dust particles
This paper presents the first results from a comparison of Planck dust maps at 353, 545 and 857GHz, ...
Aims. 3D tomography of the interstellar dust and gas may be useful in many respects, from the physic...
It is well known that the sight line toward HD 204827 in the cluster Trumpler 37 shows a UV extincti...
We present a model for the diffuse interstellar dust that explains the observed wavelength...
Abstract. Interstellar dust is an important constituent in a galaxy. Virtually all astrophysical obs...
International audienceThis article gives an overview of the constitution, physical conditions, and o...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Debris discs are typically revealed through the presence of excess emission at infrared wavelengths....
Dust is a critical component of the universe, affecting energy flow and the dynamics of star and pla...
Debris discs are typically revealed through the presence of excess emission at infrared wavelengths....
Interstellar dust was first identified through the extinction that it causes of optical starlight. I...
Dust is a crucial component in the interstellar medium of galaxies. It regulates several physical an...
The properties of dust in the interstellar medium (ISM) nearest the Sun are poorly understood becaus...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
This paper presents the first results from a comparison of Planck dust maps at 353, 545 and 857GHz, ...
Aims. 3D tomography of the interstellar dust and gas may be useful in many respects, from the physic...
It is well known that the sight line toward HD 204827 in the cluster Trumpler 37 shows a UV extincti...
We present a model for the diffuse interstellar dust that explains the observed wavelength...
Abstract. Interstellar dust is an important constituent in a galaxy. Virtually all astrophysical obs...
International audienceThis article gives an overview of the constitution, physical conditions, and o...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Debris discs are typically revealed through the presence of excess emission at infrared wavelengths....
Dust is a critical component of the universe, affecting energy flow and the dynamics of star and pla...
Debris discs are typically revealed through the presence of excess emission at infrared wavelengths....
Interstellar dust was first identified through the extinction that it causes of optical starlight. I...
Dust is a crucial component in the interstellar medium of galaxies. It regulates several physical an...
The properties of dust in the interstellar medium (ISM) nearest the Sun are poorly understood becaus...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
This paper presents the first results from a comparison of Planck dust maps at 353, 545 and 857GHz, ...
Aims. 3D tomography of the interstellar dust and gas may be useful in many respects, from the physic...
It is well known that the sight line toward HD 204827 in the cluster Trumpler 37 shows a UV extincti...