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UID:9a08672ba8294d46ecbe8ed30058a82e
CATEGORIES:Guest Speaker Night
CREATED:20210404T175050
SUMMARY:Guest Speaker - Dr Maria Cunningham - UNSW
LOCATION:: Online
DESCRIPTION:Understanding how stars form - new information from large radio surveysGala
 xies are the building blocks of the Universe. Stars, in their births and de
 aths, shape galaxy evolution, and hence understanding how stars form is imp
 ortant.\nAs stars form deep in molecular clouds, we can only observe the pr
 ocess of their formation at radio wavelengths, which are transparent to the
  dust that molecular clouds contain.\nIn this talk I will explain how star 
 formation works, what we do and do not know, and how large-scale automated 
 telescope surveys coupled with automated analysis techniques are driving fo
 rward our understanding of star formation and galaxy evolution.\nDr Maria C
 unninghamI gained my PhD jointly with CSIRO ATNF and what is now WSU. While
  undertaking my PhD I also ran the Public Access Observatory of WSU, at the
  Werrington North campus. In 2002 I accepted a lectureship at UNSW, in the 
 School of Physics, and there I have stayed. I have been lucky enough to use
  some of the world's premier research facilities, such as the Atacama Large
  Millimetre Array ALMA. However, I have a strong interest in both teaching 
 and research, and I am pretty handy with teaching-level optical telescopes 
 on a cold clear night. They are invaluable for interesting students in scie
 nce.\n
X-ALT-DESC;FMTTYPE=text/html:<h2>Understanding how stars form - new information from large radio surveys
 </h2><p>Galaxies are the building blocks of the Universe. Stars, in their b
 irths and deaths, shape galaxy evolution, and hence understanding how stars
  form is important.</p><p>As stars form deep in molecular clouds, we can on
 ly observe the process of their formation at radio wavelengths, which are t
 ransparent to the dust that molecular clouds contain.</p><p>In this talk I 
 will explain how star formation works, what we do and do not know, and how 
 large-scale automated telescope surveys coupled with automated analysis tec
 hniques are driving forward our understanding of star formation and galaxy 
 evolution.</p><h2><img src="https://www.sasi.net.au/images/articles/Dr_Mari
 a_Cunningham.jpg" alt="Dr Maria Cunningham" style="margin-right: 10px; floa
 t: left;" />Dr Maria Cunningham</h2><p>I gained my PhD jointly with CSIRO A
 TNF and what is now WSU. While undertaking my PhD I also ran the Public Acc
 ess Observatory of WSU, at the Werrington North campus. In 2002 I accepted 
 a lectureship at UNSW, in the School of Physics, and there I have stayed. I
  have been lucky enough to use some of the world's premier research facilit
 ies, such as the Atacama Large Millimetre Array ALMA. However, I have a str
 ong interest in both teaching and research, and I am pretty handy with teac
 hing-level optical telescopes on a cold clear night. They are invaluable fo
 r interesting students in science.</p>
DTSTAMP:20260620T160228
DTSTART;TZID=Australia/Sydney:20210902T193000
DTEND;TZID=Australia/Sydney:20210902T213000
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