... The dust emits continuum excess above the stellar photosphere, while the gas is traced by atomic and molecular lines over a wide range of wavelengths. ...
... Both events were recorded in a narrow CVF filter at 3.55 micron, where the light is expected to come from the stellar photosphere without any contamination by atonic or molecular lines. ...
... Janssen, K. & Cauzzi, G. 2006, Astronomy and Astrophysics Dynamics of the solar photosphere with IBIS. ... I. Reversed intensity structure in the mid-photosphere . Last Updated: 04 May, 2004 .. ...
... Solar moss isn't found growing only on the Sun's north side, but as a rule seems to lie above the photosphere or visible surface, in the transition region of the solar atmosphere. ...
... The observations with SOHO's Michelson Doppler Imager (MDI) provided long-duration, highly detailed, and well calibrated time- lapse movies of the magnetic fields on the visible surface or "photosphere" of the Sun. ...
... Penza, V., Caccin, B., Cauzzi, G. , Falchi, A. , Falciani, R., Smaldone L.A.: 2003, Possible Lines for the Diagnostics of the Deep Photosphere with IBIS , Proc. Themis Atelier , Toulouse April 2002, ed. J. Arnaud, in press . ...
... in excess of that due to the photosphere has been detected in the near (Oasa et al ... mid-infrared, because the stellar photosphere overwhelms the disk emission in the ... BD disks 605 Fig. 6. Disk and photosphere predicted SEDs. ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/bd_roph/bd_roph.pdf -- 1910.5 Кб -- 11.09.2007 Похожие документы
... Below ё4 Їm, the emission is dominated by the stellar photosphere, assumed here as a black body at T? . ... infer the existence of disks from nearinfrared photometry, where the emission is largely dominated by the stellar photosphere ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/bd_disk_cha/ms.ps.gz -- 82.3 Кб -- 11.09.2007 Похожие документы