AD Leo observed with Chandra LETG: emission measure distribution density, and element abundances of the coronal plasma
A. Maggio(Osservatorio Astronomico di Palermo), S. S. Murray(Center for Astrophysics Harvard & Smithsonian), V. Kashyap(Center for Astrophysics Harvard & Smithsonian), G. Micela(Osservatorio Astronomico di Palermo), F. R. Harnden(Smithsonian Astrophysical Observatory), J. J. Drake(Lockheed Martin (United States)), G. Pérès(AgroParisTech), S. Sciortino(Osservatorio Astronomico di Palermo)
Unknown
December 1, 2002
Cited by 3
Related Papers
Statistics, Handle with Care: Detecting Multiple Model Components with the Likelihood Ratio Test
|The Astrophysical Journal|2002|696
The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
|Astronomy and Astrophysics|2006|366
A Wavelet-Based Algorithm for the Spatial Analysis of Poisson Data
|Unknown|2001|353
The<i>Gaia</i>-ESO Survey: the Galactic thick to thin disc transition
|Astronomy and Astrophysics|2014|241
Ten Simple Rules for the Care and Feeding of Scientific Data
|PLoS Computational Biology|2014|240