Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S292(8), p. 285-285, 2012
DOI: 10.1017/s1743921313001397
Full text: Unavailable
AbstractI summarize a recent study scrutinizing the various sources of uncertainties in estimating the dust mass of a galaxy. These effects are demonstrated on the Herschel observations of the Large Magellanic Cloud.