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Monday, November 1st at 2.00pm @ the JAC

  Padelis Papadopoulos

ETH Zurich

CI as a new H2 mass tracer: the case for Ultra Luminous Infrared Galaxies (ULIRGs)

  ABSTRACT: I will discuss recent results that show the CI J=1--0 line at 492 GHz to be a potent and even better H2 gas mass tracer than 12CO, 13CO especially at ULIRGs. Implication about gas mass tracing in the high-z Universe will be briefly discussed.


Contact: Chris Davis. Updated: Thu Oct 7 08:26:48 HST 2004

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