<html><head><meta http-equiv="Content-Type" content="text/html charset=utf-8"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space;" class=""><div class="">Dear all, </div><div class=""><div class=""><br class=""></div><div class="">Astro Journal club starts on Wednesday at 3 p.m. (sharp) in the seminar room F-201 of the Physics Department. </div><div class=""><br class=""></div><div class="">Presenter: Ivan Delvecchio, dr. sc.</div><div class=""><br class=""></div><div class="">Title: An intermediate-mass black hole in the centre of the globular cluster 47 Tucanae</div><div class=""><br class=""></div>Authors: Kiziltan et al. (2017)<br class=""><br class=""><div class="">Abstract: </div><div class=""><div class="">Intermediate mass black holes play a critical role in understanding the evolutionary connection between stellar mass and super-massive black holes. However, to date the existence of these species of black holes remains ambiguous and their formation process is therefore unknown. It has been long suspected that black holes with masses <span tabindex="0" id="MathJax-Element-1-Frame" class="MathJax"><nobr class=""><span id="MathJax-Span-1" class="math" style="width: 6.778em; display: inline-block;"><span style="display: inline-block; position: relative; width: 5.477em; height: 0px; font-size: 15px;" class=""><span style="position: absolute; clip: rect(1.547em, 1005.48em, 2.972em, -1000em); top: -2.597em; left: 0em;" class=""><span id="MathJax-Span-2" class="mrow"><span id="MathJax-Span-3" class="msubsup"><span style="display: inline-block; position: relative; width: 1.429em; height: 0px;" class=""><span style="position: absolute; clip: rect(3.163em, 1000.98em, 4.192em, -1000em); top: -4.009em; left: 0em;" class=""><span id="MathJax-Span-4" class="mn" style="font-family: STIXGeneral;">10</span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span><span style="position: absolute; top: -4.412em; left: 1em;" class=""><span id="MathJax-Span-5" class="texatom"><span id="MathJax-Span-6" class="mrow"><span id="MathJax-Span-7" class="mn" style="font-size: 10px; font-family: STIXGeneral;">2</span></span></span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span></span></span><span id="MathJax-Span-8" class="mo" style="font-family: STIXGeneral; padding-left: 0.25em;">−</span><span id="MathJax-Span-9" class="msubsup" style="padding-left: 0.25em;"><span style="display: inline-block; position: relative; width: 1.429em; height: 0px;" class=""><span style="position: absolute; clip: rect(3.163em, 1000.98em, 4.192em, -1000em); top: -4.009em; left: 0em;" class=""><span id="MathJax-Span-10" class="mn" style="font-family: STIXGeneral;">10</span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span><span style="position: absolute; top: -4.412em; left: 1em;" class=""><span id="MathJax-Span-11" class="texatom"><span id="MathJax-Span-12" class="mrow"><span id="MathJax-Span-13" class="mn" style="font-size: 10px; font-family: STIXGeneral;">4</span></span></span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span></span></span><span id="MathJax-Span-14" class="msubsup"><span style="display: inline-block; position: relative; width: 1.447em; height: 0px;" class=""><span style="position: absolute; clip: rect(3.186em, 1000.87em, 4.178em, -1000em); top: -4.009em; left: 0em;" class=""><span id="MathJax-Span-15" class="mi" style="font-family: STIXGeneral; font-style: italic;">M<span style="display: inline-block; overflow: hidden; height: 1px; width: 0.039em;" class=""></span></span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span><span style="position: absolute; top: -3.859em; left: 0.833em;" class=""><span id="MathJax-Span-16" class="texatom"><span id="MathJax-Span-17" class="mrow"><span id="MathJax-Span-18" class="mo" style="font-size: 10px; font-family: STIXGeneral;">⊙</span></span></span><span style="display: inline-block; width: 0px; height: 4.009em;" class=""></span></span></span></span></span><span style="display: inline-block; width: 0px; height: 2.597em;" class=""></span></span></span><span style="display: inline-block; overflow: hidden; vertical-align: -0.323em; border-left-width: 0px; border-left-style: solid; width: 0px; height: 1.476em;" class=""></span></span></nobr></span> should form and reside in dense stellar systems. Therefore, dedicated observational campaigns have targeted globular cluster for many decades searching for signatures of these elusive objects. All candidates found in these targeted searches appear radio dim and do not have the X-ray to radio flux ratio predicted by the fundamental plane for accreting black holes. Based on the lack of an electromagnetic counterpart upper limits of <span tabindex="0" id="MathJax-Element-2-Frame" class="MathJax"><nobr class=""><span id="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