Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...
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... Великолепная семерка" - это семь радиотихих близких одиночных нейтронных звезд , открытых спутником РОСАТ. Первый объект, звезда Волтера , был открыт в 1996 г. То что это одиночная близкая нейтронная звезда стало ясно практически сразу по экстремально большому отношению рентгеновского потока к оптическому. ... В стандартных моделях затухания поля в коре нейтронных звезд получается, что чем горячее звезда, тем быстрее затухает поле (это связано с худшей проводимостью коры более горячего объекта). ...
... The mount is also adjustable so you can orient the axis of rotation to make it parallel with the Earth's axis of rotation (see the section on Polar Alignment). ... Locate the opening in the equatorial mount on the DEC axis. ... To mount the telescope tube: 1. ... ADJUSTING THE MOUNT FOR POLAR ALIGNMENT In order for the clock drive to track accurately, the telescope's axis of rotation must be parallel to the Earth's axis of rotation, a process known as polar alignment. ... R.A. & DEC axis ! ...
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Ссылки http://www.princetonastronomy.org/papers/losmandy_manual.pdf -- 177.1 Кб -- 16.03.2004 Похожие документы
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