1,721,702 research outputs found

    Oral History Interview of Leo T. Crismon

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    A transcription of ARCH CA 9-10, an interview of retired seminary librarian Leo T. Crismon by Tom Sherwood, recorded Oct. 20 & 24, 1978. Transcribed by Michele Fowler

    Letter from Leo T. Wontkowski to Fr. Pelkington

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    Providence College Department of Theater, Dance & Film Mark Twain Tonight Letter from Leo T. Wontkowski, Principal of Dighton Junior High School, North Dighton, Mass. to Fr. Pelkington May 15, 1972https://digitalcommons.providence.edu/marktwain_commentary/1000/thumbnail.jp

    Leo T. Lynn

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    Theoretical Design and Actual Tests of the Heating and Ventilating Systems of the Catholic University Gymnasium and Annex

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    by Cyril J. Corwin and Leo T. O'Connor.Typescript.Thesis (B.S.E.--Mechanical)--Catholic University of America, 1922

    Oral history interview with Leo T. Zbanek

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    Planning and building the new center

    Leo T Dissected with the MUSE-Faint Survey

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    Leo T is the lowest mass galaxy known to contain neutral gas and to show signs of recent star formation, which makes it a valuable laboratory for studying the nature of gas and star formation at the limits of where galaxies are found to have rejuvenating episodes of star formation. Here we discuss a novel study of Leo T that uses data from the MUSE integral field spectrograph and photometric data from HST. The high sensitivity of MUSE allowed us to increase the number of Leo T stars observed spectroscopically from 19 to 75. We studied the age and metallicity of these stars and identified two populations, all consistent with similar metallicity of [Fe/H] \sim -1.5 dex, suggesting that a large fraction of metals were ejected. Within the young population, we discovered three emission line Be stars, supporting the conclusion that rapidly rotating massive stars are common in metal-poor environments. We find differences in the dynamics of young and old stars, with the young population having a velocity dispersion consistent with the kinematics of the cold component of the neutral gas. This finding directly links the recent star formation in Leo T with the cold component of the neutral gas.Comment: 6 pages, 6 figures. Accepted for publication in the proceedings of IAU Symposium 379: Dynamical Masses of Local Group Galaxies. Based on source article arXiv:2308.1626

    Ruther, Leo T. J. (Birth, 1912-01-25)

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    Address: 4060 Runnymede457/1912Original record filed in drawer labeled 'Runk-Ryan'

    Deep HI observations of Leo T with WSRT

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    VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Deep neutral hydrogen observations of Leo T with the Westerbork Synthesis Radio Telescope.' (bibcode: 2018A&A...612A..26A
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