Dusty stellar nurseries from the dark side of a galaxy

April 18, 2012 By Dr. Holly Thomas
Left-hand panel: The red colors in this image show the galaxy M66 as it appears at the sub-mm wavelength of 850 microns, while the white background shows the galaxy as it appears in visible light. Regions of cold dust that appear as dark streaks in the white image glow brightly in the red image. Right-hand panel: The SCUBA-2 image at 850 microns seen on its own. Credit: VLT/ESO, JAC, G. Bendo

(Phys.org) -- A new multi-million pound camera is producing its first detailed pictures of our neighboring galaxies, revealing vast, dusty stellar nurseries where the next generation of stars is being created. "This exquisite image from the galaxy M66 in the constellation Leo is exactly the promising start we were hoping for," said Dr. Stephen Serjeant, the team's co-leader from The Open University. "This is a wonderfully exciting taste of things to come."

When looking up at the Milky Way, an irregular pattern of dark regions obscures the light of the stars. The dark patches are caused by trailing through the and blocking out the starlight; they contain vast stellar nurseries where the next generation of stars is being created. These dark lanes are not exclusive to the Milky Way, but can be found in all spiral galaxies.

Although they are dark to our eyes, these dust lanes actually glow brightly at sub-millimetre (sub-mm) wavelengths. A revolutionary new camera, called SCUBA-2, is ideally suited to detect this long-wavelength . It is mounted on the world's largest sub-mm telescope, the 15-metre James Clerk Maxwell Telescope (JCMT) in Hawaii, and is the most powerful camera ever developed for observing sub-mm wavelengths. It detects 1000 times longer than human eyes can see.

The James Clerk Maxwell Telescope is situated at 14,000 feet atop Mauna Kea in Hawaii. Credit: Nik Szymanek.

This image promises to be the first of many stunning results from the JCMT Legacy Survey (NGLS). The main aim of the survey is to understand how the broader environment of a galaxy affects its gas and dust content. For example, galaxies in dense clusters can lose their gas and dust through interactions with other galaxies in the cluster or simply by the head wind they feel while moving through the hot gas trapped inside the cluster. The NGLS is an led by astronomers from Canada, the Netherlands, and the United Kingdom which is using SCUBA-2 to observe 150 galaxies in the local universe.

The NGLS team has spent much of the last five years studying molecular hydrogen emission using another instrument on the JCMT. "It is very exciting to now see the first results from the SCUBA-2 side of our program starting to come in," says Professor Christine Wilson, the Principal Investigator from McMaster University in Canada. "We have a unique sample of galaxies that we are studying and having SCUBA-2 data will let us measure their gas and dust content. Gas and dust usually go hand-in-hand in galaxies, but from time to time, you find a surprise."

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not rated yet Apr 18, 2012
It looks like pictures for the first two illustrations were mistakenly lifted from an earlier PO article. The galaxy shown in the the first picture is M51 and both pictures appeared in an earlier 2011 piece about the SCUBA-2 camera: http://phys.org/n...ide.html

Here's a link to the press release containing the new images of M66 described in the captions above: http://outreach.j...2-S2NGS/
not rated yet Apr 18, 2012
"Left-hand panel: The red colors in this image show the galaxy M66 as it appears at the sub-mm wavelength of 850 microns, the white background shows the galaxy as it appears in visible light."

Physorg, come on!!! You are doing an increasingly poor job of providing these snippets, even when all you do is translate a press release. There is no "left panel" here.

Get your act together and hire some editors. This is becoming increasingly ridiculous.
1 / 5 (5) Apr 18, 2012
Even more apparent is that the galaxy is growing rather than contracting, through division/spawning new cores. In this case, the two major outside cores seem to have grown more massive through time as they migrate closer to the central core, leaving dusty lanes in their orbital wakes. And the southern compact cloud is likely another core forming in the early stages of LaViolette's continuous creation model.
1 / 5 (5) Apr 18, 2012
Hi. Looking at that picture, it seems like an active galactic nucleus with jets which terminate where the surrounding gas and dust etc causes the jets to 'shock' and slow and shed energy which allows more aggregation and phase changes which result in star formation conditions/content. The arcing streams is obviously the equatorial 'spiral arms' from those jet-terminations which are skewed around by the frame-dragging and other accretion-disc and re-entering/arcing and inflow processes/forces associated with the formation of the galactic nucleus etc. That's what it looks like to me, anyhow. Cheers!

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