ar X iv : a st ro - p h / 97 10 35 9 v 1 3 1 O ct 1 99 7 A SEARCH FOR SOLAR - LIKE OSCILLATIONS IN α Cen A
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چکیده
We have been using a new method to search for solar-like oscillations that involves measuring temperature changes via their effect on the equivalent widths of the Balmer hydrogen lines. We observed α Cen A over six nights in 1995 with the 3.9-metre Anglo-Australian Telescope and the European Southern Observatory's 3.6-metre telescope in Chile. Oscillations were not detected, with an upper limit only slightly higher than the expected signal.
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ar X iv : a st ro - p h / 97 10 36 7 v 1 3 1 O ct 1 99 7 Geometrical parametrization of warps for edge - on galaxies
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ar X iv : a st ro - p h / 02 09 35 9 v 1 1 8 Se p 20 02 Oscillations in α Cen A observed with UCLES at the AAT
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متن کامل
35 9 v 2 3 D ec 1 99 7 A SEARCH FOR SOLAR - LIKE OSCILLATIONS IN α Cen A
We have been using a new method to search for solar-like oscillations that involves measuring temperature changes via their effect on the equivalent widths of the Balmer hydrogen lines. We observed α Cen A over six nights in 1995 with the 3.9-metre Anglo-Australian Telescope and the Eu-ropean Southern Observatory's 3.6-metre telescope in Chile. Oscillations were not detected, with an upper limi...
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B, V and R optical photometry performed on the field of the GRB 970111 soon after its detection by BeppoSAX is presented. No remarkable optical object is found inside the corrected error box. The optical counterpart of an X–ray and radio source and a suspected red variable (probably an eclipsing binary) have been detected inside the field of GRB 970111.
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تاریخ انتشار 1997