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dc.contributor.authorBergner, J.B.
dc.contributor.authorShirley, Y.L.
dc.contributor.authorJørgensen, J.K.
dc.contributor.authorMcGuire, B.
dc.contributor.authorAalto, S.
dc.contributor.authorAnderson, C.M.
dc.contributor.authorChin, G.
dc.contributor.authorGerin, M.
dc.contributor.authorHartogh, P.
dc.contributor.authorKim, D.
dc.contributor.authorLeisawitz, D.
dc.contributor.authorNajita, J.
dc.contributor.authorSchwarz, K.R.
dc.contributor.authorTielens, A.G.G.M.
dc.contributor.authorWalker, C.K.
dc.contributor.authorWilner, D.J.
dc.contributor.authorWollack, E.J.
dc.date.accessioned2022-03-18T00:03:45Z
dc.date.available2022-03-18T00:03:45Z
dc.date.issued2022
dc.identifier.citationBergner, J. B., Shirley, Y. L., Jørgensen, J. K., McGuire, B., Aalto, S., Anderson, C. M., Chin, G., Gerin, M., Hartogh, P., Kim, D., Leisawitz, D., Najita, J., Schwarz, K. R., Tielens, A. G. G. M., Walker, C. K., Wilner, D. J., & Wollack, E. J. (2022). Astrochemistry With the Orbiting Astronomical Satellite for Investigating Stellar Systems. Frontiers in Astronomy and Space Sciences.
dc.identifier.issn2296-987X
dc.identifier.doi10.3389/fspas.2021.793922
dc.identifier.urihttp://hdl.handle.net/10150/663649
dc.description.abstractChemistry 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. Copyright © 2022 Bergner, Shirley, Jørgensen, McGuire, Aalto, Anderson, Chin, Gerin, Hartogh, Kim, Leisawitz, Najita, Schwarz, Tielens, Walker, Wilner and Wollack.
dc.language.isoen
dc.publisherFrontiers Media S.A.
dc.rightsCopyright © 2022 Bergner, Shirley, Jørgensen, McGuire, Aalto, Anderson, Chin, Gerin, Hartogh, Kim, Leisawitz, Najita, Schwarz, Tielens, Walker, Wilner and Wollack. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY).
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectastrochemistry
dc.subjectfar-infrared astronomy
dc.subjectinterstellar molecules
dc.subjectspace telescopes
dc.subjectstar-forming regions
dc.titleAstrochemistry With the Orbiting Astronomical Satellite for Investigating Stellar Systems
dc.typeArticle
dc.typetext
dc.contributor.departmentDepartment of Astronomy, University of Arizona
dc.contributor.departmentSteward Observatory, University of Arizona
dc.contributor.departmentWyant College of Optical Sciences, University of Arizona
dc.identifier.journalFrontiers in Astronomy and Space Sciences
dc.description.noteOpen access journal
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleFrontiers in Astronomy and Space Sciences
refterms.dateFOA2022-03-18T00:03:45Z


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Copyright © 2022 Bergner, Shirley, Jørgensen, McGuire, Aalto, Anderson, Chin, Gerin, Hartogh, Kim, Leisawitz, Najita, Schwarz, Tielens, Walker, Wilner and Wollack. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY).
Except where otherwise noted, this item's license is described as Copyright © 2022 Bergner, Shirley, Jørgensen, McGuire, Aalto, Anderson, Chin, Gerin, Hartogh, Kim, Leisawitz, Najita, Schwarz, Tielens, Walker, Wilner and Wollack. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY).