Very recent observations with the GBT reveal a far more widespread interstellar aromatic chemistry than expected at the earliest stages of star formation. Here, we wish to finish the observations we have already begun, and to substantially expand our sample size, to determine exactly how widespread the phenomenon is, not only across a variety of sources, but also across a range of evolutionary stages.
Name | Institution |
---|---|
Andrew Burkhardt | Center for Astrophysics | Harvard & Smithsonian; Wellesley College; Worcester State University |
Brett McGuire * | National Radio Astronomy Observatory; Massachusetts Institute of Technology |
Ilsa Cooke | British Columbia, University of; Rennes 1, Université de |
Tony Remijan | National Radio Astronomy Observatory |
Mark Siebert | Cornell University; Virginia, University of; Chalmers University Of Technology |
Kin Long Kelvin Lee | Massachusetts Institute of Technology; Center for Astrophysics | Harvard & Smithsonian |
CI XUE | Massachusetts Institute of Technology |
Ryan Loomis | National Radio Astronomy Observatory |
Michael McCarthy | Center for Astrophysics | Harvard & Smithsonian |
* indicates the PI