Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]Spectropolarimetric observations in the 3-micron ice band are presented for the infrared sources GL 2591, GL 2136, W 33A and Elias 29 (Rho Ophiuchi dark cloud). Some continuum polarization measurements between 1.2 and 5.0 microns are also considered. Increasing polarization with optical depth within the ice feature are observed for GL 2136 and Elias 29 confirming that there is little or no increase in the level of polarization within the same feature for GL 2591, in contrast with the polarization increases that have previously been observed for this source across the 10- and 20-micron si...
This is the improved version of the ice crystal single-scattering property dataset introduced in the...
Context. The small compact isolated dark clouds also known as “Bok globules” are believed ...
In order to understand the role of magnetic fields in the process of star formation, we require deta...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
We present spectropolarimetry of the 3.1 μm water-ice feature in the Becklin-Neugebauer (BN) object ...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
Abstract. We present optical polarimetry and high res-olution spectroscopy of a sample of stars towa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found at: http://www.nature.com/nature/index.html Copyright Nature Publishin...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
We present one of largest studies to date of combined near-infrared and submillimeter linear polariz...
This is the improved version of the ice crystal single-scattering property dataset introduced in the...
Context. The small compact isolated dark clouds also known as “Bok globules” are believed ...
In order to understand the role of magnetic fields in the process of star formation, we require deta...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing....
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
We present spectropolarimetry of the 3.1 μm water-ice feature in the Becklin-Neugebauer (BN) object ...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
Abstract. We present optical polarimetry and high res-olution spectroscopy of a sample of stars towa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found at: http://www.nature.com/nature/index.html Copyright Nature Publishin...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
We present one of largest studies to date of combined near-infrared and submillimeter linear polariz...
This is the improved version of the ice crystal single-scattering property dataset introduced in the...
Context. The small compact isolated dark clouds also known as “Bok globules” are believed ...
In order to understand the role of magnetic fields in the process of star formation, we require deta...