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Gordon Stacey’s research interests center on studies of star formation and its interplay with the interstellar medium across cosmic time. These studies have focused on far-infrared and submillimeter wavelength fine-structure and rotational line emission from abundant atoms, ions, and molecules. These lines provide the cooling mechanism by which an interstellar gas cloud can collapse to form a star, and also trace the hardness and intensity of ambient interstellar radiation fields. The hardness of the radiation field is determined by the most massive stars on the main sequence, hence the age of the stellar population, while the intensity of the radiation field is determined by the numbers of stars per unit volume, hence the intensity of star formation. Therefore, not only do these lines reveal regions of star formation, they also unveil the characteristics of the newly formed stars – their age and spatial extent.
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ASTRONOMY & ASTROPHYSICS (2024)
Fiona Harrison,Robert Kennicutt,Julianne Dalcanton, Tim De Zeeuw, Andrew Driesman,Jonathan Fortney,Gabriela Gonzalez, Jordan Goodman,Marc Kamionkowski,Bruce MacIntosh, Jacobus Oschmann,Rachel Osten,
crossref(2023)
arxiv(2022)
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI (2022)
CCAT-Prime collaboration,M. Aravena,J. E. Austermann,K. Basu,N. Battaglia,B. Beringue,F. Bertoldi,F. Bigiel,J. R. Bond,P. C. Breysse,C. Broughton,R. Bustos,
arxiv(2022)
S. K. Choi,C. J. Duell,J. Austermann,N. F. Cothard, J. Gao, R. G. Freundt,C. Groppi,T. Herter,J. Hubmayr,Z. B. Huber,B. Keller,Y. Li,
Journal of Low Temperature Physicsno. 5-6 (2022): 849-856
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI (2022)
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