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dc.contributor.authorGicquel, A.
dc.contributor.authorBauer, J.M.
dc.contributor.authorKramer, E.A.
dc.contributor.authorMainzer, A.K.
dc.contributor.authorMasiero, J.R.
dc.date.accessioned2024-03-26T06:51:27Z
dc.date.available2024-03-26T06:51:27Z
dc.date.issued2023-01-09
dc.identifier.citationAdeline Gicquel et al 2023 Planet. Sci. J. 4 3
dc.identifier.issn2632-3338
dc.identifier.doi10.3847/PSJ/aca8ac
dc.identifier.urihttp://hdl.handle.net/10150/671854
dc.description.abstractWe report on the observed fluxes of the comets detected by NEOWISE during the first year of operations after the spacecraft’s reactivation. The sample included 57 comets. Of the comets detected, 30 were short-period comets (27 Jupiter-family comets, 1 Centaur, 2 Halley-type comets), and 27 were long-period comets. From the measured fluxes in the two NEOWISE bands, proxies for the gas production and coma dust are derived. We find a relationship between heliocentric distance, perihelion distance, and the gas-to-dust proxy fractions. © 2023. The Author(s). Published by the American Astronomical Society.
dc.language.isoen
dc.publisherInstitute of Physics
dc.rights© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
dc.rights.urihttps://creativecommons.org/licenses/by/4.0
dc.titleCO and CO2 Productions Rates of Comets Observed by NEOWISE within Year 1 of the Reactivated Mission
dc.typeArticle
dc.typetext
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizona
dc.identifier.journalPlanetary Science Journal
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.journaltitlePlanetary Science Journal
refterms.dateFOA2024-03-26T06:51:27Z


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© 2023. The Author(s). Published by the American Astronomical Society.  Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.