Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(414), p. 642-651, 2011
DOI: 10.1111/j.1365-2966.2011.18429.x
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Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics
Journal article published in 2011 by
A. Cortesi 
,
M.~R R. Merrifield ,
M. Arnaboldi ,
O. Gerhard,
I. Martinez-Valpuesta,
K. Saha,
L. Coccato,
S. Bamford,
N.~R R. Napolitano ,
P. Das,
N.~G G. Douglas,
A.~J J. Romanowsky,
K. Kuijken,
M. Capaccioli,
K.~C C. Freeman
,
M.~R R. Merrifield ,
M. Arnaboldi ,
O. Gerhard,
I. Martinez-Valpuesta,
K. Saha,
L. Coccato,
S. Bamford,
N.~R R. Napolitano ,
P. Das,
N.~G G. Douglas,
A.~J J. Romanowsky,
K. Kuijken,
M. Capaccioli,
K.~C C. Freeman
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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