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"Tadpole Hunters" May Net Forming Planets
"Tadpole Hunters" May Net Forming Planets
23 May 2001
(Source: Commonwealth Scientific & Industrial Research Organisation Australia)

Commonwealth Scientific and Industrial Research Organisation Australia

Contacts:

Ms Helen Sim
Sector Communicator
Australia Telescope National Facility
PO Box 76
Marsfield NSW 1710
Phone: +61 2 9372 4251
Fax: +61 2 9372 4310
Email: hsim@atnf.csiro.au

Ms Rosie Schmedding
Communicator
CSIRO National Awareness
PO Box 225
Dickson ACT 2602
Phone:+61 2 6276 6520
Fax:+61 2 6276 6821
Mobile: +61 0418 622 653
Email: Rosie.Schmedding@nap.csiro.au

Ref 2001/122

Researchers using CSIRO's Australia Telescope have found they can spot the dusty blobs that might be planet systems in the making.

This will help astronomers hunt more effectively for these elusive objects, and better estimate how many planet-forming systems are out there.

"We were very surprised that we could see these blobs," says Dr B=E4rbel Koribalski of CSIRO's Australia Telescope National Facility. "It goes against the predictions."

Planet formation is a common process in the Universe, astronomers think. Planets and their parent stars are born from compact clouds of gas and dust. But very few of these have been found.

In 1994 the Hubble Space Telescope saw blobs of gas and dust in a star-forming region in the constellation of Orion. They were dubbed protoplanetary disks, or 'proplyds' for short. Each is thought to hide a forming star, with material around it that could later form planets.

Last year astronomers using the Hubble Space Telescope (HST) announced they had found three of the blobs on the outskirts of a region in our Galaxy where many stars are forming. Called NGC 3603, the region lies 20,000 light-years away in the Southern constellation of Carina.

A team led by Anita M=FCcke of the University of Montreal was independently using CSIRO's Australia Telescope to study massive stars in the same region. Tipped off by the optical studies, they scanned their data for the objects and found them there, unexpectedly bright.

Later, they found a fourth object that had not been picked up in the original HST study.

Apart from the objects in Orion and NGC 3603, only two other proplyds have been found.

There may be many reasons for this apparent scarcity.

Optical telescopes can see proplyds only when they are lying against a brightly lit background.

Many proplyds may have been mistaken for other kinds of objects - in particular, small blobs of glowing hydrogen gas called 'ultracompact HII regions'.

Astronomers detect a lot of those blobs - about four times as many as star-formation theories predict.

"It seems likely that many are really proplyds instead," says Dr Koribalski.

Just as radiation from the Sun blasts material from a comet into a sweeping tail, strong UV radiation from nearby hot young stars shapes the proplyds into sleek tadpole forms.

"We will be able to look through our catalogues of radio sources for tadpole-shaped objects," Dr Koribalski says. "Many of them may turn out to be proplyds. To confirm that, we'd get optical images of them to check that they have that tadpole shape."

The sizes of the proplyds may also make them hard to identify.

"The objects in NGC 3603 are much bigger than the proplyds in Orion. If you put the small Orion proplyds in NGC 3603, which is much further out, you wouldn't be able to see them," says Dr Koribalski.

On the other hand, if we saw the NGC 3603 proplyds closer, at the distance of the Orion nebula, "they wouldn't look like blobs at all - they might look like huge pillars of gas and dust," she adds.

But proplyds may also be genuinely scarce. The blasts of radiation that give them their tadpole shape may also destroy them before they can form planets.

A finding announced on 1 May at the Spring meeting of the American Physical Society notes that 90 percent of the proplyds in Orion will be destroyed in the next several hundred thousand years.

"NGC 3603 has about 100 times the ionizing power of the comparable region in Orion," says Dr M=FCcke. "The proplyds there may be blasted away by radiation long before they get a chance to form planetary systems."

The members of the observing team are Dr Anita M=FCcke(University of Montreal), Dr B=E4rbel Koribalski (CSIRO Australia Telescope National Facility), Dr Tony Moffat (University of Montreal), Dr Mike Corcoran (NASA Goddard Space Flight Center), and Dr Ian Stevens (University of Birmingham, UK).

More information:

Dr B=E4rbel Koribalski, CSIRO Australia Telescope National Facility
02-9372-4361, bkoribal@atnf.csiro.au

Dr Anita M=FCcke, University of Montreal
+1-514-343-6111 ext 4681, muecke@astro.umontreal.ca

IMAGE CAPTIONS:
[Image 1: http://www.csiro.au/page.asp?type=3DimageDef&id=3DNGC3603HST]
Researchers using CSIRO's Australia Telescope have found they can spot the dusty blobs that might be planet systems in the making. Credit: Wolfgang Brandner (ESO), Eva K. Grebel (MPIA Heidelberg)

[Image 2: http://www.csiro.au/images/mediaReleases/NGC3603med.jpg]
The green contour lines are an Australia Telescope radio image of the star- forming region NGC 3603. They are overlaid on HST images of the same region. The blobs that may be forming star-systems are marked as P1, P2, P3 and P4. Their tadpole shape is not apparent at this scale but can be seen in close-ups. Credit: radio image, A . M=FCcke, B. Koribalski, A.F.J. Moffat, M.F. Corcoran, I.R. Stevens. HST image, Credit: W. Brandner, E.K. Grebel, You-Hua Chu and NASA.

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Last Updated: 5 Jun 2001