2022ApJ...940L..26T


Query : 2022ApJ...940L..26T

2022ApJ...940L..26T - Astrophys. J., 940, L26 (2022/November-3)

Mid-infrared Polarization of the Diffuse Interstellar Medium toward CygOB2-12.

TELESCO C.M., VAROSI F., WRIGHT C., DRAINE B.T., FERNANDEZ ACOSTA S.J. and PACKHAM C.

Abstract (from CDS):

We present the first mid-IR detection of the linear polarization toward the star CygOB2-12, a luminous blue hypergiant that, with AV ≈ 10 mag of foreground extinction, is a benchmark in the study of the properties of dust in the diffuse interstellar medium. The 8-13 μm spectropolarimetry, obtained with the CanariCam multimode camera at the Gran Telescopio CANARIAS shows clear trends with wavelength characteristic of silicate grains aligned in the interstellar magnetic field. The maximum polarization, detected with 7.8σ statistical significance near 10.2 μm, is (1.24 ± 0.28)% with position angle 126° ± 8°. We comment on these measurements in the context of recent models for the dust composition in the diffuse interstellar medium.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Diffuse interstellar clouds - Spectropolarimetry - Silicate grains

VizieR on-line data: <Available at CDS (J/ApJ/940/L26): fig1.dat fig2.dat>

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 WR 48a WR* 13 12 39.6052790136 -62 42 55.939362876       16.081   WC6 106 0
2 WR 112 WR* 18 16 33.4909366272 -18 58 42.341845368   20.7 17.7     WC8+O6/7III/V 143 0
3 * d Cyg PM* 19 50 37.7235287221 +52 59 16.790345304 7.84 6.31 5.03     K3IIICN2 183 0
4 RAFGL 2591 Y*O 20 29 24.8230 +40 11 19.590           ~ 640 0
5 Schulte 12 s*b 20 32 40.9572199728 +41 14 29.279036940 16.1 14.45 11.702     B3-4Ia+ 453 0
6 * 5 Lac s*r 22 29 31.8281552924 +47 42 24.861238614 7.15 6.05 4.37 2.98 1.91 K9Ia+B2V 152 0

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