Poster Open Access
Greco, Jennifer J.;
Cushing, Michael C.
{ "inLanguage": { "alternateName": "eng", "@type": "Language", "name": "English" }, "description": "<p>Brown dwarfs are substellar objects too low mass to initiate the hydrogen fusion necessary to be considered stars. Ultracool dwarfs, objects with spectral types of M7 or later, are a mix of low mass stars and brown dwarfs. We have obtained the first high-resolution (R ∼ 45, 000) H- and K-band spectral sequence of ultracool dwarfs with spectral types ranging from M1.5 V to T6, including known low-gravity objects at six spectral types (M9, L0, L1, L2, L3, L5). All spectra were obtained using the Immersion Grating INfrared Spectrometer (IGRINS) at a resolving power of R ∼ 45,000. We compared 22 of our objects to synthetic spectra created from the atmospheric models of Saumon & Marley (2008), to measure specific properties including effective temperature, cloud properties, rotational velocities, and surface gravity.</p>", "license": "https://creativecommons.org/licenses/by/4.0/legalcode", "creator": [ { "affiliation": "Uppsala University/SCAS", "@id": "https://orcid.org/0000-0002-4649-1568", "@type": "Person", "name": "Greco, Jennifer J." }, { "affiliation": "University of Toledo", "@id": "https://orcid.org/0000-0001-7780-3352", "@type": "Person", "name": "Cushing, Michael C." } ], "url": "https://zenodo.org/record/4564681", "datePublished": "2021-02-26", "@type": "CreativeWork", "keywords": [ "low-mass stars", "substellar objects", "ultracool dwarfs", "spectroscopy", "near-infrared spectroscopy" ], "@context": "https://schema.org/", "identifier": "https://doi.org/10.5281/zenodo.4564681", "@id": "https://doi.org/10.5281/zenodo.4564681", "workFeatured": { "url": "http://coolstars20.cfa.harvard.edu/cs20half", "alternateName": "CS20.5", "location": "virtual", "@type": "Event", "name": "The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun" }, "name": "A High Resolution H- and K-Band Spectroscopic Sequence of Ultracool Dwarfs" }
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