Vast Filament of Star-Forming Gas Spans 50 Light Years

“But ammonia is an excellent tracer of dense, star-forming gas,” says Friesen, “and these large ammonia maps will allow us to track the motions and temperature of the densest gas. This is critical to assessing whether gas clouds and filaments are stable, or are undergoing collapse on their way to forming new stars.”

The image accompanies the first release of results from the collaboration’s Green Bank Ammonia Survey (GAS), published in the Astrophysical Journal. The collaboration’s other co-Principal Investigator is Jaime Pineda, from the Max Planck Institute for Extraterrestrial Physics; the team also includes astronomers from the University of Toronto’s Department of Astronomy & Astrophysics and Canadian Institute for Theoretical Astrophysics.

The goal of GAS is to survey all the major, nearby star-forming regions in the northern half of the Gould Belt — a ring of young stars and gas clouds that circles the entire sky and runs through the constellation Orion. The survey will eventually provide a clearer picture over a larger portion of the sky of the temperatures and motions of gas within these dynamic stellar nurseries.

Notes:
1) The first GAS data release includes data from observations of four Gould Belt clouds: B18 in the constellation Taurus; NGC 1333 in Perseus; L1688 in Ophiuchus; and Orion A North in Orion.

2) The 100-metre Green Bank Telescope is located in the National Radio Quiet Zone, a 34 thousand square kilometre area in which radio transmissions are tightly restricted. The Green Bank Observatory (GBO) is a facility of the National Science Foundation operated under a cooperative agreement by Associated Universities, Inc.

Contacts and sources:
Rachel Friesen, Dunlap Fellow
Dunlap Institute for Astronomy & Astrophysics
University of Toronto

 

Citation: The Green Bank Ammonia Survey (GAS): First Results of NH3 Mapping the Gould Belt: https://arxiv.org/abs/1704.06318