The increased number of high-frequency (> 30 GHz) radio observations are unveiling the complexity and diversity of radio spectra among (and within) galaxies, along with the associated difficulties in interpreting such measurements. We propose to address this by using 14hr of GBT time to create MUSTANG-2/90GHz maps for more than ~30 star-forming regions within a representative sub-sample of 12 late-type galaxies included in the Star Formation in Radio Survey (SFRS). When complemented with existing VLA 3, 15, and 33GHz data from SFRS, these new MUSTANG-2 data will critically pin down the spectra where nearly pure free-free emission is expected, allowing us to create robust spectral index maps and properly separate free-free emission from other components (i.e., synchrotron, AME, and thermal dust) on sub-kpc scales. Given the wealth of existing space- and ground-based ancillary data for these sources, these new 90GHz maps will allow us to (1) characterize the physical conditions for star formation in a large, heterogenous sample, (2) help unveil the physics of anomalous microwave emission for existing and new detections, and (3) create a library of radio spectra on sub-kpc scales that will be critical for interpreting radio spectra of high-z objects, where less data is available.
Name | Institution |
---|---|
Eric Murphy * | National Radio Astronomy Observatory; Virginia, University of; California Institute of Technology |
Brian Mason | National Radio Astronomy Observatory |
Sean Linden | Arizona, University of |
Charles Romero | Pennsylvania, University of; Virginia, University of; Center for Astrophysics | Harvard & Smithsonian |
Tony Mroczkowski | European Southern Observatory; Institut de Ciències de l'Espai |
Simon Dicker | Pennsylvania, University of |
Eric Faustino Jimnez-Andrade | México, Universidad Nacional Autónoma de |
Jean Turner | California at Los Angeles, University of; California at Los Angeles, University of |
Abigail Harden | Agnes Scott College |
Emmanuel Momjian | National Radio Astronomy Observatory |
Brandon Hensley | Princeton University |
Eva Schinnerer | National Radio Astronomy Observatory; Max-Planck-Institut für Astronomie |
Bruce Draine | Princeton University |
Mark Devlin | Pennsylvania, University of |
Sara Stanchfield | Pennsylvania, University of |
Jonathan Sievers | Toronto, University of; McGill University; Princeton University; KwaZulu-Natal, University of |
Dillon Dong | National Radio Astronomy Observatory; California Institute of Technology |
* indicates the PI