2014A&A...569L...1A


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.31CET17:52:30

2014A&A...569L...1A - Astronomy and Astrophysics, volume 569, L1-1 (2014/9-1)

On the radiation driven alignment of dust grains: Detection of the polarization hole in a starless core.

ALVES F.O., FRAU P., GIRART J.M., FRANCO G.A.P., SANTOS F.P. and WIESEMEYER H.

Abstract (from CDS):

We aim to investigate the polarization properties of a starless core in an early evolutionary stage. Linear polarization data reveal the properties of the dust grains in the distinct phases of the interstellar medium. Our goal is to investigate how the polarization degree and angle correlate with the cloud and core gas. We use optical, near infrared, and submillimeter polarization observations on the starless object Pipe-109 in the Pipe nebula. Our data cover a physical scale range of 0.08 to 0.4pc, comprising the dense gas, envelope, and the surrounding cloud. The cloud polarization is well traced by the optical data. The near infrared polarization is produced by a mixed population of grains from the core border and the cloud gas. The optical and near infrared polarization toward the cloud reaches the maximum possible value and saturates with respect to the visual extinction. The core polarization is predominantly traced by the submillimeter data and has a steep decrease with respect to the visual extinction. Modeling of the submillimeter polarization indicates a magnetic field main direction projected onto the plane-of-sky and loss of grain alignment for densities higher than 6x104cm–3 (or AV>30mag). The object is immersed in a magnetized medium with a very ordered magnetic field. The absence of internal source of radiation significantly affects the polarization efficiencies in the core, creating a polarization hole at the center of the starless core. This result supports the theory of dust grain alignment via radiative torques

Abstract Copyright:

Journal keyword(s): stars: formation - ISM: magnetic fields - techniques: polarimetric - ISM: individual objects: Core 109

VizieR on-line data: <Available at CDS (J/A+A/569/L1): opt.dat nir.dat submm.dat list.dat fits/*>

Errata: + corrigendum vol. 574, p. C4 (2015)

Simbad objects: 4

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Number of rows : 4

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NAME Perseus Cloud SFR 03 35.0 +31 13           ~ 1086 0
2 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 3546 0
3 NAME the Pipe Nebula DNe 17 30 -25.0           ~ 339 1
4 DCld 001.6+03.8 DNe 17 35 47.50 -25 32 59.0           ~ 53 0

    Equat.    Gal    SGal    Ecl

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2020.10.31-17:52:30

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