Bradley E. Schaefer

Results: 7



#Item
1KIC8462852 Faded at an Average Rate of 0.165±0.013 Magnitudes Per Century From 1890 To 1989 Bradley E. Schaefer arXiv:1601.03256v1 [astro-ph.SR] 13 Jan 2016

KIC8462852 Faded at an Average Rate of 0.165±0.013 Magnitudes Per Century From 1890 To 1989 Bradley E. Schaefer arXiv:1601.03256v1 [astro-ph.SR] 13 Jan 2016

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Source URL: arxiv.org

- Date: 2016-01-13 20:23:11
    2Short-Duration Flares on Mira Stars Bradley E. Schaefer ([removed]) Louisiana State University Mira stars are slowly pulsating red giant stars with periods of order a year, so it came as a startling surprise when

    Short-Duration Flares on Mira Stars Bradley E. Schaefer ([removed]) Louisiana State University Mira stars are slowly pulsating red giant stars with periods of order a year, so it came as a startling surprise when

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    Source URL: keplerscience.arc.nasa.gov

    Language: English - Date: 2014-08-23 20:44:59
    3A Planet Around the Dwarf Nova V893 Sco? Bradley E. Schaefer, [removed], Louisiana State University The dwarf nova system V893 Sco shows eclipses, and very accurate groundbased eclipse timing has shown that there

    A Planet Around the Dwarf Nova V893 Sco? Bradley E. Schaefer, [removed], Louisiana State University The dwarf nova system V893 Sco shows eclipses, and very accurate groundbased eclipse timing has shown that there

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    Source URL: keplerscience.arc.nasa.gov

    Language: English - Date: 2014-08-23 20:44:59
    4High-Precision Eclipse Timings of Recurrent Nova U Scorpii Bradley E. Schaefer, [removed], Louisiana State University Recurrent nova (RN) U Scorpii (U Sco) is the prototype RN, with ten known thermonuclear eruptio

    High-Precision Eclipse Timings of Recurrent Nova U Scorpii Bradley E. Schaefer, [removed], Louisiana State University Recurrent nova (RN) U Scorpii (U Sco) is the prototype RN, with ten known thermonuclear eruptio

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    Source URL: keplerscience.arc.nasa.gov

    Language: English - Date: 2014-08-23 20:44:59
    5Short-Duration Flares on Mira Stars Bradley E. Schaefer Department of Physics & Astronomy, Louisiana State University ([removed]) Mira stars are slowly pulsating red giant stars with periods of order a year, so it

    Short-Duration Flares on Mira Stars Bradley E. Schaefer Department of Physics & Astronomy, Louisiana State University ([removed]) Mira stars are slowly pulsating red giant stars with periods of order a year, so it

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    Source URL: keplerscience.arc.nasa.gov

    Language: English - Date: 2014-02-03 01:26:42
    6Abstract from the American Astronomical Society meeting in San Diego, California, for talk[removed]on 10 January 2005

    Abstract from the American Astronomical Society meeting in San Diego, California, for talk[removed]on 10 January 2005

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    Source URL: www.phys.lsu.edu

    Language: English - Date: 2005-01-03 10:34:52
    7JHA, xxxvi[removed]THE EPOCH OF THE CONSTELLATIONS ON THE FARNESE

    JHA, xxxvi[removed]THE EPOCH OF THE CONSTELLATIONS ON THE FARNESE

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    Source URL: www.phys.lsu.edu

    Language: English - Date: 2005-02-25 10:27:00