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astro-phastro-ph.SRastro-ph.EPastro-ph.IM

On Valency

published · living versions
W_3tjd289h·v1 · currentpublished

Preprints & journals

15 papers in the corpus · 2005–2012
Planetary companions around the metal-poor star HIP 119521208.4000v1 · J. Setiawan, V. Roccatagliata, D. Fedele et al.2012 · 9 citationsA&A 540, 141, 2012
Optical spectroscopy of EX Lupi during quiescence and outburst: Infall, wind, and dynamics in the accretion flow1206.3081v1 · Aurora Sicilia-Aguilar, 'Agnes K'osp'al, Johny Setiawan et al.2012 · 67 citationsarXiv
Rotational velocities of nearby young stars1005.0984v1 · Patrick Weise, Ralf Launhardt, Johny Setiawan et al.2010 · 72 citationsarXiv
New Herbig Ae/Be stars confirmed via high-resolution optical spectroscopy1004.3386v1 · A. Carmona, M.E. van den Ancker, M. Audard et al.2010 · 39 citationsarXiv
EX Lupi in quiescence0906.3168v1 · N. Sipos, P. 'Abrah'am, J. Acosta-Pulido et al.2009 · 68 citationsarXiv
Testing planet formation theories with Giant stars0801.3336v1 · Luca Pasquini, M.P. Doellinger, A. Hatzes et al.2008 · 5 citationsarXiv
A young massive planet in a star-disk system.18172492 · Setiawan, J, Henning, Th, Launhardt, R et al.2008 · 147 citationsNature. 2008;451(7174):38-41
Evolved stars hint to an external origin of enhanced metallicity in planet-hosting stars0707.0788v1 · L. Pasquini, M.P. Doellinger, A. Weiss et al.2007 · 163 citationsarXiv
Planets around active stars0704.2145v1 · J. Setiawan, P. Weise, Th. Henning et al.2007 · 31 citationsarXiv
Physical parameters of evolved stars in clusters and in the field from line-depth ratios0704.1462v1 · K. Biazzo, L. Pasquini, A. Frasca et al.2007 · 0 citationsarXiv
Basic physical parameters of a selected sample of evolved starsastro-ph/0608160v2 · L. da Silva, L. Girardi, L. Pasquini et al.2006 · 492 citationsarXiv
A substellar companion around the intermediate-mass giant star HD 11977astro-ph/0505510v1 · J. Setiawan, J. Rodmann, L. da Silva et al.2005 · 97 citationsarXiv
Career total: 53 works. 15 are in this corpus.

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