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X-WR-CALNAME;VALUE=TEXT:The Ph.D. colloquium by Sumin Tang: Exploring the Long-term and Extreme Variability of Stars
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SUMMARY:The Ph.D. colloquium by Sumin Tang: Exploring the Long-term and Extreme Variability of Stars
DESCRIPTION:<p><span lang="en-us"><span style="font-family: 'Times New Roman';"><span lang="en-us"><strong><span><span lang="en-us"><span>The Ph.D. colloquium by</span></span><span lang="en-us"></span><span lang="en-us"></span><span lang="en-us"> <span>Sumin Tang</span></span></span></strong></span></span></span></p><p><span lang="en-us"><span style="font-family: 'Times New Roman';"><span lang="en-us"><strong><span>Talk Title</span></strong></span><span lang="en-us"></span><span lang="en-us"></span><span lang="en-us"><span>: Exploring the Long-term and Extreme Variability of Stars<br></span></span></span></span><strong><span lang="en-us"><span style="font-family: 'Times New Roman';"><span lang="en-us">Location: </span></span></span></strong><span lang="en-us"><span style="font-family: 'Times New Roman';"><span lang="en-us">Phillips Auditorium</span></span></span></p><p><span lang="en-us"><span style="font-family: 'Times New Roman';">Following her colloquium, Sumin will defend her thesis in the same room.</span></span></p><p><span lang="en-us"><strong><span style="font-family: 'Times New Roman';">Abstract</span></strong></span><span lang="en-us"></span><span lang="en-us"></span><span lang="en-us"><span style="font-family: 'Times New Roman';">:</span></span><span lang="en-us"></span><span lang="en-us"></span><span lang="en-us"> <span style="font-family: 'Times New Roman';">Exploring the Long-term and Extreme Variability of Stars</span></span></p><p><span lang="en-us"><span style="font-family: 'Times New Roman';">Stellar variations over decades are poorly explored. With the unique 100 yr coverage of DASCH (Digital Acess to a Sky Century@Harvard), for the first time, we are able to study the variable sky over long timescales in a systematic way. I have discovered exciting new types of long-term variables, which do not match any of the common classes. The most interesting one to date is a peculiar 10-yr nova. With P=119 days, it is interestingly located in the gap region between classic novae and symbiotic novae. The most probable explanation of the outburst is Hydrogen shell-burning on the WD without significant mass loss, which suggests a promising new channel for Type Ia Supernovae (SNe). We have found peculiar long-term K giant variables with 1-2 mag slow variations over decades. Most of them show strong Ca H&amp;K emission, and 5 of them are covered by Kepler and show (in 4 stars) star spots and flaring activities. This suggests that the mysterious long-term variations may be related to strong star spots and magnetic activities which may be a new mechanism for dust formation or ejection. We discovered a 5-yr dust accretion event in KU Cyg, which is probably linked with its accretion disk. I conclude my thesis with the DASCH-Kepler variable catalog. Compared with the ASAS variable catalog, I recovered most of large amplitude variable stars (&gt;0.5 mag). Other post-thesis discoveries include an Epsilon Aurigae-like object, and a new class of CV with stellar magnetic cycle driven accretion.</span></span></p>
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STATUS:CONFIRMED
DTSTART:20120502T140000Z
DTEND:20120502T153000Z
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