An international team of astronomers led by Texas Tech University scientist Dr. Christopher Britt has spotted a very young star, called CXOGBS J173643.8-282122 (CX330 for short), in an area away from where stars normally form.
Comparison of CX330 brightness before (left) and after outburst. Image credit: C.T. Britt et al.
CX330 was detected as an X-ray source in 2009 by NASA’s Chandra X-Ray Observatory while surveying the bulge in the central region of the Milky Way.
Further observations indicated this object was emitting optical light as well. With only these clues, scientists had no idea what this object was.
But when Dr. Britt and co-authors examined infrared images of the same area taken with NASA’s Wide-field Infrared Survey Explorer (WISE), they realized this object has a lot of warm dust around it, which must have been heated by an outburst.
Comparing WISE data from 2010 with Spitzer Space Telescope data from 2007, they determined CX330 likely is a young star that has been outbursting for several years. In fact, in that three-year period, its brightness had increased a few hundred times.
The team gathered data about the star from a variety of other observatories, including the ground-based SOAR, Magellan, and Gemini telescopes. They also measured the intensity of light emitted from CX330. By combining the different perspectives on the object, a clearer picture emerged.
“We tried various interpretations for it, and the only one that makes sense is that this rapidly growing young star is forming in the middle of nowhere,” Dr. Britt said.
CX330’s behavior is remarkably similar to FU Orionis, a young outbursting star that had an initial three-month outburst in 1936-37 and whose bright emissions have been fading ever since. CX330 is fading as well, but its brightness hasn’t fallen more than a factor of 10 since its peak in 2010 or 2011.
This star is more compact, hotter and likely more massive than the FU Orionis-like objects, launching faster outflows slamming into the gas and dust around it.
“The disk has probably heated to the point where the gas in the disk has become ionized, leading to a rapid increase in how fast the material falls onto the star,” said team member Dr. Tom Maccarone, also from Texas Tech University.
Most puzzling to the team, FU Orionis and the stars like it – there are only about 10 of them – are located in starburst regions.
That’s because young stars form and feed from their surroundings, which are the gas- and dust-rich regions in star-forming clouds.
By contrast, the region of star formation closest to CX330 is several hundred light-years away. If our Sun were this isolated, the nearest star-forming region would be near Orion.
“CX330 is both more intense and more isolated than any of these young outbursting objects that we’ve ever seen,” said team member Dr. Joel Green, from the Space Telescope Science Institute.
“This could be the tip of the iceberg – these objects may be everywhere.”
In fact, it is possible all stars go through this dramatic stage of development in their youth, but many of the outbursts are too short in cosmological time for humans to observe.
How did CX330 become so isolated? The scientists aren’t sure.
One idea is that this star was born in a star-forming region but was ejected into its present lonely pocket of our Galaxy.
“This is unlikely,” the astronomers said. “Because CX330 is in a youthful phase of its development – likely less than 1 million years old – and still is eating its surrounding disk, it must have formed near its present location in the sky.”
“If it had migrated from a star-forming region, it couldn’t get there in its lifetime without stripping its disk away entirely.”
CX330 also may help scientists study how stars form under different circumstances.
One scenario suggests stars form through turbulence. In this ‘hierarchical’ model, a critical density of gas in a cloud causes the cloud to gravitationally collapse into a star.
A different model, called ‘competitive accretion,’ claims stars begin as low-mass cores that fight over the mass of material left in the cloud.
CX330 more naturally fits into the first scenario, as the turbulent circumstances would theoretically allow for a lone star to form.
It is still possible other intermediate- to low-mass stars are in the immediate vicinity of CX330 but have not been detected yet.
The team’s findings will be published in the August 11, 2016 issue of the Monthly Notices of the Royal Astronomical Society (arXiv.org preprint).
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C.T. Britt et al. 2016. Discovery of a Long-Lived, High Amplitude Dusty Infrared Transient. MNRAS 460 (3): 2822-2833; doi: 10.1093/mnras/stw1182
