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<div style="font-family:"Segoe UI",Helvetica,Arial,sans-serif"><span id="docs-internal-guid-86d1851e-9600-8d8e-733d-c5fa57d08efb" style=""><span id="docs-internal-guid-9e838874-b9fd-c26f-7292-368ffed344e3" style="">
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<div style="text-align:center"><span style="font-family:Cambria; background-color:rgb(255,255,255); vertical-align:baseline; white-space:pre-wrap"><span id="docs-internal-guid-748f50ce-f689-54d2-9b41-5a3c77a9e486" style=""><span id="docs-internal-guid-44741882-f788-0e32-c8e8-2b168c3681ef" style=""><span id="docs-internal-guid-d5bed97d-3f42-6ae7-0034-104ccf7b3897" style=""><span id="docs-internal-guid-498729f8-679a-0a20-28d6-2d9b55698270" style=""><span id="docs-internal-guid-51391753-8bcf-ef16-57fc-e1b7affdfc5f" style=""><span id="docs-internal-guid-42e41036-7fff-21b4-7d44-d4dd211c366f" style=""><span id="docs-internal-guid-5f05f5c9-7fff-beba-2406-c965c2ae057c" style=""><span id="docs-internal-guid-b54610e0-7fff-3506-dfd5-090d1f414dc8" style=""><span id="docs-internal-guid-bccd1570-7fff-2f10-1577-65d92a6f7f88" style=""><span id="docs-internal-guid-6ebcb931-7fff-a406-6f79-0c1a1a112fad" style=""><span id="docs-internal-guid-d24e26c2-7fff-11b0-b0a7-4af97d505a88"><span id="docs-internal-guid-ae6f7d9c-7fff-2c60-55cd-30fef3f73124">
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 28pt; color: rgb(192, 0, 0); background-color: transparent; font-weight: 700; vertical-align: baseline;">Fall 2018 Colloquium</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 16pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Department of Physics & Astronomy, TAMU-Commerce</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 16pt; color: rgb(192, 0, 0); background-color: transparent; font-weight: 700; vertical-align: baseline;">Oct 18, Thursday, 4-5 PM in Science Building 127</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; background-color: transparent; vertical-align: baseline;">(coffee and cookies will be served at 3:50 PM)</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; color: rgb(0, 176, 80); background-color: transparent; font-weight: 700; vertical-align: baseline;">Astrophysics</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;">Supermassive Black Holes in Nearby Galaxies</span><span style="font-size: 18pt; color: rgb(0, 0, 255); background-color: transparent; font-weight: 700; vertical-align: baseline;"><br class="kix-line-break">
</span><span style="font-size: 14pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Dr. Jonelle Walsh</span></p>
<p dir="ltr" style="line-height: 1.38; margin-top: 0pt; margin-bottom: 0pt;"><span style="font-size: 14pt; color: rgb(11, 83, 148); background-color: transparent; font-weight: 700; vertical-align: baseline;">Texas A&M University at College Station</span><span style="font-size: 14pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">
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<img src="https://lh5.googleusercontent.com/vgqjMURjGWstA-tB8EVOVivRoqCRF9rM58owEqx5I3CBgybMJJ4HBCSd4A5B7YQBxARLwu8PJn4OrbExRGNE7pyvQUanaSP0Q67BXJabOL8yOIbXajGYbiUOmNvzt1Us9sGlQxJh" width="152" height="174" style="border: none; transform: rotate(0.00rad); -webkit-transform: rotate(0.00rad);">
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<span style="font-size: 11pt; vertical-align: baseline;">Dr. Jonelle Walsh earned a B.A. (2005) in Physics from Bowdoin College, and M.S. (2007) and Ph.D. (2011) degrees in Physics from the University of California, Irvine. She spent three years as a National
Science Foundation Astronomy and Astrophysics Postdoctoral Fellow at the University of Texas, Austin, and three years as a Mitchell Postdoctoral Fellow in Astronomy at Texas A&M University, College Station. In 2017, Dr. Walsh began her appointment as an assistant
professor at Texas A&M, where she is currently doing research in astrophysics. Her research focuses on studying supermassive black holes in nearby galaxies with the goal of understanding how black holes and their host galaxies form and evolve together. More
information about Dr. Walsh and her research can be found at </span><a href="https://urldefense.proofpoint.com/v2/url?u=http-3A__jonellewalsh.weebly.com&d=DwMFAw&c=oqyuZuih6ykib6aKiBq22_bich4AVfYGoLertJN0bEc&r=hjwEO_XYlnwAQWUGeaCrW47w4mK-Al28-BKyRvaivBs&m=o8nkESfQgMpZxkWTKUEhkiZn66KeW_-iRTy7A-TDlfw&s=BNy39lcBNE1SVYuM70AZthIDYu9E2JPleU_qAnKbjk4&e=" style="text-decoration-line: none;"><span style="font-size: 11pt; color: rgb(17, 85, 204); text-decoration-line: underline; vertical-align: baseline;">https://jonellewalsh.weebly.com</span></a></p>
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<p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:4pt;"><span style="font-size: 12pt; background-color: transparent; font-weight: 700; vertical-align: baseline;">Abstract</span></p>
<p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt;text-align: justify;">
<span style="font-size: 12pt; font-family: Arial; background-color: transparent; vertical-align: baseline;">Over the past 15 years it has become increasingly clear that supermassive (greater than a million solar mass) black holes are essential components of
galaxies, as demonstrated by the empirical correlations connecting black hole masses and large-scale galaxy properties. Although about ~100 dynamical black hole mass measurements have been made to date, the local black hole mass census is highly incomplete.
Gaining a more complete picture of black hole demographics and a deeper understanding of the mechanisms that drive black hole/galaxy evolution requires the measurement of black holes in a wider range of galaxy types with diverse evolutionary histories. In
this talk, I will discuss the measurement of black holes in an exciting population of local galaxies that show remarkable similarities to galaxies observed at earlier epochs in the Universe. I will also describe a Gemini Large and Long Program aimed at addressing
a bias in the types of galaxies for which dynamical black hole mass measurements have been made.</span></p>
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