Sky and Telescope - October 2015 - 29

DIGITIZED SKY SURVEY 2

T. PILLAI & J. KAUFFMAN, SOURCES: SPITZER
GLIMPSE & MIPSGAL IMAGES, CSO HERTZ DATA

"Brick"
Galactic Center
50 light-years

T. PILLAI & J. KAUFFMAN, SOURCES:
SPITZER GLIMPSE & MIPSGAL IMAGES,
JCMT SCUPOL DATA

BRICK & SNAKE Two dense molecular clouds known as the
Brick (top) and the Snake (bottom) show up as dark shadows in
Spitzer images (left), silhouetted against a background of midinfrared emission from warm dust and gas. But the clouds glow
at submillimeter (top right) and far-infrared wavelengths (bottom
right). The polarization of this long-wavelength radiation showed
Pillai's team how the magnetic field is oriented: parallel to the
Brick filament and perpendicular to the Snake filament.

IN ANOTHER
LIGHT
The L1495/B213
filaments of cold,
dense gas are
just shadows in
the visible-light
Digitized Sky
Survey image
(above), but they
glow gently at
submillimeter
wavelengths
(left).

ESO / APEX / A. HACAR ET AL. / DIGITIZED SKY SURVEY 2

isn't to say measurements are impossible: for example,
strong magnetic fields can split a spectral line into
multiple lines at slightly different wavelengths (known as
the Zeeman effect), and the direction of a cloud's magnetic field will influence the polarization of light passing
through it, which astronomers can then measure.
The problem is that magnetic fields suff use the
sparse gas that floats between stars and star-forming
clouds. In that drifting, low-density gas, the magnetic
field is weak but well aligned. So if astronomers observe
the magnetic field in a collapsing cloud, their view
would also include the gas between Earth and the cloud.
Chances are this interstellar gas will dominate their
measurements and perhaps even give a false sense of
what the magnetic field looks like within the cloud.
But astronomers never shy away from a challenge.
Thushara Pillai (Max Planck Institute for Radio Astronomy, Germany) and colleagues zeroed in on two of
the darkest infrared shadows along the galactic plane.
Dubbed the Brick and the Snake, these clouds lie 12,000
and 27,000 light-years from Earth, respectively.
Though the shadows are dark in the infrared, they
glow gently at even longer wavelengths. Dust grains, especially well-aligned ones on the clouds' surfaces, polarize
this radiation as it escapes. Pillai's team used archival data
from the James Clerk Maxwell Telescope and the Caltech

"Snake"

30 light-years

Sk yandTelescope.com October 2015

29


http://www.SkyandTelescope.com

Sky and Telescope - October 2015

Table of Contents for the Digital Edition of Sky and Telescope - October 2015

Contents
Sky and Telescope - October 2015 - Cover1
Sky and Telescope - October 2015 - Cover2
Sky and Telescope - October 2015 - 1
Sky and Telescope - October 2015 - Contents
Sky and Telescope - October 2015 - 3
Sky and Telescope - October 2015 - A
Sky and Telescope - October 2015 - B
Sky and Telescope - October 2015 - 4
Sky and Telescope - October 2015 - 5
Sky and Telescope - October 2015 - 6
Sky and Telescope - October 2015 - 7
Sky and Telescope - October 2015 - 8
Sky and Telescope - October 2015 - 9
Sky and Telescope - October 2015 - 10
Sky and Telescope - October 2015 - 11
Sky and Telescope - October 2015 - 12
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Sky and Telescope - October 2015 - 15
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Sky and Telescope - October 2015 - 17
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Sky and Telescope - October 2015 - 24
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Sky and Telescope - October 2015 - 29
Sky and Telescope - October 2015 - 30
Sky and Telescope - October 2015 - 31
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Sky and Telescope - October 2015 - 33
Sky and Telescope - October 2015 - 34
Sky and Telescope - October 2015 - 35
Sky and Telescope - October 2015 - 36
Sky and Telescope - October 2015 - 37
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Sky and Telescope - October 2015 - 40
Sky and Telescope - October 2015 - 41
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Sky and Telescope - October 2015 - Cover3
Sky and Telescope - October 2015 - Cover4
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