... В теме В разделе По форуму . ... Научная панорама ? arxiv:1507.05823 Ушедшие без взрыва . ... arxiv:1507.05823 Ушедшие без взрыва: обзор архивных данных КТХ по поиску исчезнувших массивных звезд (Gone without a bang: An archival HST survey for disappearing massive stars) . ... Это примерно то, что и ожидалось, т.е., пусть и на очень низкой статистике, но подтверждает идею о "тихом коллапсе" заметной доли массивных звезд. http://xray.sai.msu.ru/~polar/sci_rev/327.html#arxiv/1507.05823 . ...

Меркурий . ... Фотографии . ... Страница: История "Mariner-10" , КА "Messenger" NASA , 1-я встреча Messenger , Итог 1-я встречи , 2-я встреча Messenger , 3-я встреча Messenger , Выход на орбиту , Полгода на Меркурии , Год на орбите , Быть или не быть? ... Космический аппарат "MESSENGER" . ... Отдельная страница/ссылка на новость: Карта Бетховена, Меркурий . Краткое описание картинки: . ... Обилие калия и тория на поверхности Меркурия установлено гамма-спектрометром космического аппарата MESSENGER. ...

... Moon Phase below . ... ARTICLE: Why the moon always shows us the same face . ... Before you continue reading, you should know that this was not always the case, i.e. the Moon once was rotating with respect to the Earth, so that on every night a terrestrial observer (if there was one, because this was long, long before mankind appeared on our planet, and even before any major animals had appeared) saw another face of the Moon. ... Figure 1 (not to scale) shows how we can imagine the system Earth-Moon...

... Публикации: "Odessa Astronomical Publications", 1997, vol. ... There are four basic forms (REGISTRATION, HOTEL RESERVATION, PAPER % CONTRIBUTION and PAYMENT) to be completed and returned to the CONTACT % ADDRESS mentioned below. ... SUMMER SCHOOL 10 Dundee Remote Sensing Summer School 49 Scottish Universities Summer School in Physics Physical Processes in the Coastal Zone: Computer Modelling and Remote Sensing 12th August to 29th August 1997. ...

The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...

... On the basis of hypothesis about Solar s ystem formating from endo-Galactic Vortex, stated by е.л. Trunaev, who have acquainted the author of the present work with his manuscript in 1991 during personal contact , the results of attempt to apply its main rules to some calculations at the Solar system actually and at planets satellite systems are below stated. ... orbit in . ... All satellite systems of planets, as well as the Solar system, are formed from two- branch pre-planetary (pre-Solar)...

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

This page is devoted to information on Supernova 1999by in NGC 2841 . ... When I got back I discovered this SN backed up in my e-mail folder. 1999by was discovered by both Ron Arbour and the Lick Observatory Supernova Search team while it was still getting brighter. ... ErnТ BerkС CCD Photos page has a number of 1999by images. Konkoly Observatory 1999by images . ... Finder Charts: . ... Masao Funada finder chart showing stars in NGC 2841 w/ 1999by . ... vsnet-chart 151 ] Chart of SN1999by . ...

. Comment on J1842+7946 . Comparing the brightnesses of the two main features seen in our 5 GHz image with higher frequency VLBI images available in the literature (at 8.4 GHz from the USNO database and at 15 GHz by Kellermann et al. (1998)), one can conclude that the NW component has a steeper spectrum since the SE one becomes relatively stronger as the observing frequency increases. VLBApls home page . Last modified: 16 Oct 2000