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<div>Dear all:</div>
<div>Resend with picture and abstract. &nbsp;Dr. Whelan will be arriving around 2pm tomorrow. &nbsp;If anybody would like to meet with him, please contact me. &nbsp;We’ll also be taking him to dinner. &nbsp;Austin College is just an hour away in Sherman, TX.</div>
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<div><b class=""><font size="4" class="">Colloquium</font></b><br class="">
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<p class="MsoNormal" style="margin-bottom: 12pt;"><b class=""><span style="color: rgb(0, 176, 80);" class=""><font size="4" class="">Oct. 15, Thursday, 4-5pm in Science 127 (coffee and cookies served at 3:50pm)<br class="">
</font></span></b><b class=""><i class=""><font size="4" class="">All students currently enrolled in Physics 401 and 501 are required to atte<span style="color: rgb(31, 73, 125);" class="">n</span>d all colloquia</font><span style="color: rgb(31, 73, 125); font-size: 16pt;" class=""></span></i></b></p>
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<b class=""><font color="#0000ff" class="" size="4">A Campaign to Spectroscopically Monitor B-Type Emission-Line Stars: Year One</font></b></p>
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<b class=""><font color="#993300" class="">Prof. David G. Whelan, Austin College</font></b></p>
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<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Dr. David G. Whelan is in his second year on the faculty at Austin College. An</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">astrophysicist, he earned his Ph.D. in 2013 from the University of Virginia. He is</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">part of the Apache Point Observatory Galactic Evolution Experiment (APOGEE)</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">team, one of the four surveys currently being conducted as part of the Sloan</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Digital Sky Survey (SDSS). His primary research interests are on the nature of</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">massive stars and their impact on the interstellar medium. At Austin College, Dr.</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Whelan works with undergraduate students at the new Adams Observatory's</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">24-inch telescope to study a sample of new Be stars that were discovered with</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">APOGEE.</div>
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<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Abstract:</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Beginning in 2011, the Apache Point Observatory Galactic Evolution Experiment (APOGEE)</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">began a spectroscopic campaign to study the history of the Milky Way Galaxy. During the first three</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">years of observations, APOGEE revealed 128 previously unknown emission-line B-type stars (Be</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">stars), and observed a further 110 known Be stars. This is the largest near-infrared high-resolution</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">spectroscopic and multi-epoch dataset of Be stars in existence. APOGEE-2, which began observing in</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">2014, is making additional contributions to the original dataset.</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">As part of a campaign to determine the spectroscopic characteristics of the objects in this</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">sample, our group has undertaken a systematic program to observe this sample at optical wavelengths.</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">Many of our optical spectra have been taken at larger telescopes, but a growing number of optical</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">spectra have been taken with the Adams Observatory, Austin College. Undergraduate students are</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">taking part in every aspect of the project from sample selection to data collection and reduction, and</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">then the analysis of these data.</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">I will highlight certain discoveries made using the APOGEE sample, as well as some surprises</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">from the optical follow-up. Plans for future work will be brought up, including some more directed</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">work on Be stars in clusters with APOGEE-2, as well as what we are developing at Adams Observatory</div>
<div style="font-size: 12px; margin: 0px; font-family: Helvetica;" class="">to make efficient use of our time and resources.</div>
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