Coupled Evolutions of the Stellar Obliquity, Orbital Distance, and Planet's Radius due to the Ohmic Dissipation Induced in a Diamagnetic Hot Jupiter around a Magnetic T Tauri Star

Please use this identifier to cite or link to this item: http://ir.sinica.edu.tw/handle/201000000A/52825

Title:	Coupled Evolutions of the Stellar Obliquity, Orbital Distance, and Planet's Radius due to the Ohmic Dissipation Induced in a Diamagnetic Hot Jupiter around a Magnetic T Tauri Star
Authors:	Chang, Y-L Bodenheimer, PH Gu, P-G
Issue Date:	2012-10-01
Relation:	ASTROPHYSICAL JOURNAL 757(2), 118
URI:	http://ir.sinica.edu.tw/handle/201000000A/52825
ISSN:	http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-637X&DestApp=JCR&RQ=IF_CAT_BOXPLOT
URL:	http://adsabs.harvard.edu/abs/2012ApJ...757..118C
Appears in Collections:	天文及天文物理研究所

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