Next: Summary Up: The Epsilon Aurigae Previous: Eclipse Lightcurves for . In this section, we attempt to account for the observed asymmetry in absorption line profiles by using a crude model of the thermal expansion of the outer edge of the disk as it rotates into the radiation field of the primary. ... Hinkle and Simon (1987) proposed that the asymmetries in the pre- and post-central eclipse line profiles are a consequence of the vaporization of grains caused by heating from the primary. ...

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... A. M. M. Scaife, E. I. Curtis , M. L. Davies and 15 others. ... MNRAS , 2010, accepted . PDF | ADS | astro-ph . ... A submillimetre survey of the kinematics of the Perseus molecular cloud - III. ... MNRAS , 2010, in press . ... Citations 1 | ... MNRAS , 2010, 408, 1516 . ... The JCMT legacy survey of the Gould Belt: a first look at Serpens with HARP . ... MNRAS , 2010, 405, 759 . ... MNRAS , 2010, 402, 603 . ... PDF Star Formation in Perseus Observed with HARP . ... 2010 Emily Curtis | ...

... This is usually defined as the direction pointing toward the center of the primary body. ... NODE: The place where the plane of one orbit crosses the plane of another. ... ORBITAL PLANE: The flat surface that would result if every point on the orbit of a body was connected to the center of its primary. ... PENUMBRA: The edge of the primary body's shadow. ... PERIOD : The time required for one body to orbit the primary body. ... PROBE: A vessel designed to pass and observe an astronomical object. ...

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JSC History . ... The Archive database can be searched only to the folder level. ... The Archive database is the hard copy History Office archival guide pages. ... Note: the number of pages in the search results depends on how many records containing the search criteria are returned combined with the number of records per page requested in the 'Max Page" box (default is 100). ... Reset - removes all check marks made to the select boxes (to the left of the Record Number) on the search results page. ...

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