Doctor of Philosophy, University of Toledo, 2020, Physics
We present the results of two near-infrared spectroscopic studies of ultracool dwarfs. The first utilizes low-resolution spectroscopy to follow-up discoveries from an all-sky proper motion survey conducted using multi-epoch data from the Wide-field Infrared Survey Explorer. Using the data from NEOWISE, along with the AllWISE catalog, Schneider et al. 2016 conducted an all-sky proper motion survey to search for nearby objects with high proper motions. We present follow-up spectra of 65 of their discoveries, focusing on potentially nearby objects (d < 25 pc), candidate late-type brown dwarfs (> L7), and subdwarf candidates. We found 31 new M dwarfs, 18 new L dwarfs, and 11 new T dwarfs. Of these, 13 are subdwarfs, including one new sdL1 and two new sdL7s. Eleven of these discoveries, with spectral types ranging from M7 to T7 (including one subdwarf) are predicted to be within 25 pc, adding to the number of known objects in the solar neighborhood. The second project presents 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 and Marley 2008, fitting both the whole K-band (2.05--2.35 μm) and the CO band (2.27--2.35 μm) and obtained values of Teff, log g, vsini, vrad, and fsed for each of our objects from both sets of fits. When comparing these values with expected trends from the literature, we find some agreement, and some discrepancies. In particular we find that our Teff values are high compared to values calculated using bolometric luminosities, and our vsini values are high compared to previously published values for the same objects. Comparing the log g values for our field and low (open full item for complete abstract)
Committee: Michael C Cushing (Committee Chair); Jon Bjorkman (Committee Member); Rupali Chandar (Committee Member); Kathy Shan (Committee Member); Michael Line (Committee Member)
Subjects: Astronomy; Astrophysics; Physics