Cosmic Collision: Space Nessie Spawns Newborn Star

Deep in the depths of our galactic ocean, astronomers have observed triggered star formation in the Nessie Nebula.

Nessie’s legendary shape, revealed in an image from the Spitzer Telescope. The expanding bubble is the yellow, ring-shaped object at the far right. Credit: NASA/JPL-Caltech/Univ. Of Wisconsin.

A gaseous strand of cosmic gas and dust forms the core of the sinuous “Nessie” filament, an Infrared Dark Cloud (IRDC). This cold, dense, opaque cloud is primed to form new stars. “The gravity in this dense filament primes it to collapse into stars. If a hot star is born in the filament, it forms an expanding bubble that can collide with the filament and send it over the edge to form a new star.  The first luminous star is the first domino falling, setting off a chain reaction. As new stars form along the filament, they can trigger subsequent star formation in sequence that propagates along the filament.   The energy produced by the new stars forms new hot, expanding bubbles, colliding with pockets of cold gas in the filament, pushing the filament’s gas at the collision site over the edge to trigger even more star formation, falling like dominoes down the line.”

Using data from SOFIA, the Australia Telescope Compact Array, and the Mopra Telescope, an international team of astronomers have evidence of this triggered star formation caused by a bubble-filament interaction.

This phenomenon was revealed by observing the most luminous protostar in the region, AGAL337.916-00.477. This newly formed star was located precisely at the intersection between an expanding HII bubble and the IRDC filament. 

Data from NASA/SOFIA and CSIRO/ATCA, image credit J.Jackson

This tear-dropped shaped bubble along Nessie’s western edge is the location of high energy star clusters, compact H II regions, and, tellingly, a luminous young protostar. Both ammonia (3,3) (observed with the Australia Telescope Compact Array) and SiO 2-1 emission (observed with the Mopra Telescope) show emission peaks exactly coincident with the luminous protostar.   Both the ammonia (3,3)  and the SiO emission are unambiguous signs of the bubble slamming into the filament.

Adds Jim Jackson, Director of the Green Bank Observatory, and a lead author on this research, “We’ve known for some time that Nessie is the birthplace of stars. We’ve wondered about whether an older generation of stars can trigger the birth of new stars in a filamentary cloud.  With these data, we can see the triggering process in action. ”

This news was shared at a press conference on Tuesday, June 6th, 10:15AM MT, at the 242nd summer meeting of the American Astronomical Society. Please find a recording here.

SOFIA was a joint project of NASA and the German Space Agency at DLR. DLR provided the telescope, scheduled aircraft maintenance, and other support for the mission. NASA’s Ames Research Center in California’s Silicon Valley managed the SOFIA program, science, and mission operations in cooperation with the Universities Space Research Association, headquartered in Washington, DC  and the German SOFIA Institute at the University of Stuttgart. The aircraft was maintained and operated by NASA’s Armstrong Flight Research Center Building 703, in Palmdale, California. SOFIA achieved full operational capability in 2014 and concluded its final science flight on Sept. 29, 2022.

Data from this project also came from the Australia Telescope Compact Array/Australia Telescope National Facility (ATCA/ATNF.) ATCA is operated by CSIRO‘s Astronomy and Space Science division.

Jim Jackson is director of the Green Bank Observatory. The Green Bank Observatory is supported by the National Science Foundation and is operated by Associated Universities, Inc.

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