Astrochemistry With the Orbiting Astronomical Satellite for Investigating Stellar Systems
Artikel i vetenskaplig tidskrift, 2022
Chemistry along the star- and planet-formation sequence regulates how prebiotic building blocks—carriers of the elements CHNOPS—are incorporated into nascent planetesimals and planets. Spectral line observations across the electromagnetic spectrum are needed to fully characterize interstellar CHNOPS chemistry, yet to date there are only limited astrochemical constraints at THz frequencies. Here, we highlight advances to the study of CHNOPS astrochemistry that will be possible with the Orbiting Astronomical Satellite for Investigating Stellar Systems (OASIS). OASIS is a NASA mission concept for a space-based observatory that will utilize an inflatable 14-m reflector along with a heterodyne receiver system to observe at THz frequencies with unprecedented sensitivity and angular resolution. As part of a survey of H2O and HD toward ∼100 protostellar and protoplanetary disk systems, OASIS will also obtain statistical constraints on the emission of complex organics from protostellar hot corinos and envelopes as well as light hydrides including NH3 and H2S toward protoplanetary disks. Line surveys of high-mass hot cores, protostellar outflow shocks, and prestellar cores will also leverage the unique capabilities of OASIS to probe high-excitation organics and small hydrides, as is needed to fully understand the chemistry of these objects.
interstellar molecules
astrochemistry
star-forming regions
far-infrared astronomy
space telescopes
Författare
Jenny Bergner
University of Chicago
Yancy L. Shirley
University of Arizona
J. K. Jorgensen
Niels Bohr Institute
Brett McGuire
National Radio Astronomy Observatory
Massachusetts Institute of Technology (MIT)
Susanne Aalto
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Carrie M. Anderson
National Aeronautics and Space Administration (NASA)
Gordon Chin
National Aeronautics and Space Administration (NASA)
M. Gerin
Observatoire de Paris
P. Hartogh
Max-Planck-Gesellschaft
Daewook Kim
University of Arizona
David Leisawitz
National Aeronautics and Space Administration (NASA)
Joan Najita
NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab)
Kamber Schwarz
Max-Planck-Gesellschaft
Alexander G.G.M. Tielens
University of Maryland
Universiteit Leiden
Christopher K. Walker
University of Arizona
David J. Wilner
Harvard-Smithsonian Center for Astrophysics
Edward J. Wollack
National Aeronautics and Space Administration (NASA)
Frontiers in Astronomy and Space Sciences
2296987X (eISSN)
Vol. 8 793922Exploring the Hidden Dusty Nuclei of Galaxies (HIDDeN)
Europeiska forskningsrådet (ERC) (789410), 2018-10-01 -- 2023-09-30.
Ämneskategorier (SSIF 2011)
Rymd- och flygteknik
Astronomi, astrofysik och kosmologi
Atom- och molekylfysik och optik
DOI
10.3389/fspas.2021.793922