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<div>Dear all:</div>
<div>Resend with picture and abstract. Dr. Whelan will be arriving around 2pm tomorrow. If anybody would like to meet with him, please contact me. We’ll also be taking him to dinner. Austin College is just an hour away in Sherman, TX.</div>
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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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