CALIBRATING EXTINCTION-FREE STAR FORMATION RATE DIAGNOSTICS WITH 33 GHz FREE-FREE EMISSION IN NGC 6946
California Institute of Technology · National Radio Astronomy Observatory · +15 more institutions
Abstract
Using free-free emission measured in the Ka band (26-40 GHz) for 10 star-forming regions in the nearby galaxy NGC 6946, including its starbursting nucleus, we compare a number of star formation rate (SFR) diagnostics that are typically considered to be unaffected by interstellar extinction. These diagnostics include non-thermal radio (i.e., 1.4 GHz), total infrared (IR; 8-1000 üm), and warm dust (i.e., 24 üm) emission, along with hybrid indicators that attempt to account for obscured and unobscured emission from star-forming regions including Hñ + 24 üm and UV + IR measurements. The assumption is made that the 33 GHz free-free emission provides the most accurate measure of the current SFR. Among…
Citation impact
- FWCI
- 16.42
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- 100%
- References
- 130
Authors
23Topics & keywords
- Physics
- Astrophysics
- Extinction (optical mineralogy)
- Star formation
- Stars
- Galaxy
- Infrared
- Interstellar medium
- Life below water