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Dr. Paul Goldsmith is the Group Supervisor for 3266 – Structure of the Universe. His recent work has focused on observations of far-infrared fine structure lines to determine the complete structure of molecular clouds associated with star formation. He has also worked on determining time scales of cloud formation by using atomic hydrogen in molecular clouds as a tracer of their evolution and history. He has also been studying the impact of star formation on surrounding molecular cloud material via changes in abundance, heating of dust, shock waves, and other processes. He is actively involved in the development of technology for high resolution submillimeter and far-infrared spectroscopy.
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论文共 339 篇作者统计合作学者相似作者
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Ebrahim M. Al Seragi, Yashas L. Rajendra, Waleed Ahmad,Mehmet Kaynak,Paul F. Goldsmith, Saeed Zeinolabdedinzadeh
IEEE Transactions on Terahertz Science and Technologyno. 99 (2024): 1-18
RESEARCH IN ASTRONOMY AND ASTROPHYSICSno. 2 (2024)
Dario Pisanti, Ashish Goel,Gaurangi Gupta,Manan Arya, Benjamin Byron,Nacer Chahat,Joseph Lazio,Paul Goldsmith,Saptarshi Bandyopadhyay
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCESno. 2271 (2024): 20230073-20230073
ASTROPHYSICAL JOURNALno. 1 (2023): 40-40
J. Syed,H. Beuther,P. F. Goldsmith,Th. Henning, M. Heyer,R. S. Klessen,J. M. Stil, J. D. Soler,L. D. Anderson,J. S. Urquhart, M. R. Rugel,K. G. Johnston,
arXiv (Cornell University) (2023): A130-A130
AIAA SCITECH 2023 Forum (2023)
ASTROPHYSICAL JOURNALno. 2 (2023): 102-102
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