... 12, 2015 Abell 407 MAC 0300+3534 Nov 11 2009 31 Per Per Per Per Per Per Per Per Per Per Per Per Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy Galaxy 17mmT4 EF,ES, PATCH ,AV SUSP,AV ONLY ONCE OR TWICE, AGC 407 ,R=P MAC 0300+3541 Nov 11 ...

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... Характер изменения периода и амплитуды может служить основой дополнительной классификации всех полуправильных переменных звзд, поэтому информация об изменении периодов у каждой конкретной звезды является ценным научным результатом. Звезду S Per наблюдают астрономы-любители, что дат возможность получить кривую блеска за продолжительный период времени и изучить изменения амплитуды и периода. ... Период у этой звезды изменяется более чем в 2 раза, изменения периода хаотические с большим разбросом. ...

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... public class TiffDecoder . ... static int . ... Field Detail public static final int NEW_SUBFILE_TYPE . ... public static final int IMAGE_WIDTH . ... public static final int IMAGE_LENGTH . ... public static final int BITS_PER_SAMPLE . ... public static final int COMPRESSION . ... public static final int PHOTO_INTERP . ... public static final int IMAGE_DESCRIPTION . ... public static final int STRIP_OFFSETS . ... public static final int ORIENTATION . ... public static final int SAMPLES_PER_PIXEL . ...

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... in quotes) ( e.g . RA) ( e.g . Dec) ( e.g . Magnitude ) 91 lambda Cet 03:00:13.5 +08:56:41 Magnitude =4.70 theta Hyi 03:02:17.0 -71:51:55 Magnitude =5.53 92 alpha Cet 03:02:46.6 +04:07:35 Magnitude =2.53 11 tau ^3 Eri 03:02:48.6 -23:35:16 Magnitude =4.09 mu Hor 03:03:50.3 -59:42:04 Magnitude =5.11 23 gamma Per 03:05:29.4 +53:32:35 ...

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... The GW from coalescing compact binaries composed of NS and BH are the best understood of all astrophysical GW sources. A conservative lower limit to the event rate of galactic binary neutron star coalescence of about 1 per 100000 year follows from double pulsar   statistics studies (Narayan et al. ... In Figure  47 we show the rates of coalescence of binary WD and NS in a model elliptical galaxy   consisting of stars, depending on time elapsed since the (assumed instantaneous) star formation. ...

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... As proxy indicators of performance in each of the Observatory's principal areas of activity (research, education and public outreach, and heritage) records are maintained of (A) External Grant Income (per financial year); (B) the number of Refereed Journal Publications (per calendar year); (C) the number of Identified Media Citations (per calendar year); and (D) the number of Distinct e-Visitors (DeVs) to its web-sites (per calendar year). ... External . ... Grant Income . ... 2005 Required Income: ...

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... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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Глубокий ПЗС-обзор звездных скоплений h Per и Большой Туманности Ориона на Майданакской обсерватории Ибрагимов М.А. (1), Каримов Р.Г. (1) (1) Астрономический институт, Ташкент, Узбекистан Абстракт Сообщаются предварительные результаты глубоких ПЗС-мониторингов звездного скопления h Per и скопления в Большой Туманности Ориона, проведенных на 1.5м телескопе АЗТ-22 Майданакской обсерватории. ... Эти исследования проводились с той же целью, что и исследования по вышеописанному скоплению h Per. ...

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