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UID:9a08672ba8294d46ecbe8ed30058a82e
CATEGORIES:Guest Speaker Night
CREATED:20210404T175050
SUMMARY:Guest Speaker - Dr Maria Cunningham - UNSW
LOCATION:: Online
DESCRIPTION:<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="images/articles/Dr_Maria_Cunningham.jpg" alt="D
 r Maria Cunningham" style="margin-right: 10px; float: left;" />Dr Maria Cun
 ningham</h2><p>I 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, i
 n 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 tea
 ching and research, and I am pretty handy with teaching-level optical teles
 copes on a cold clear night. They are invaluable for interesting students i
 n science.</p>
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:20260620T160704
DTSTART;TZID=Australia/Sydney:20210902T193000
DTEND;TZID=Australia/Sydney:20210902T213000
SEQUENCE:0
TRANSP:OPAQUE
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