... 110-114 F5.2 mas/year s_mu_ra Error of RA proper motion 116-120 F5.2 mas/year s_mu_dec Error of Decl proper motion 122-122 I1 --- Src Proper motion source (2) 125-129 F5.2 --- Corr PM errors correlation coefficient 133-138 F6.2 mas Pi HIPPARCOS parallax 140-144 F4.2 mas Pi_err Parallax error 147-152 I6 --- Hip_no HIPPARCOS number ------------------------------------------------------------------------------- Note (1) Sources of radial velocity data: 1 Moscow group measurements (Sov.Astron.Let., ...

Name Last modified Size Description . Parent Directory 28-Dec-2015 15:33 - nsv.dat 04-Feb-2016 15:51 1.6M nsv_pos.dat 04-Feb-2016 16:30 565k readme.txt 02-Dec-2015 18:16 15k ref.txt 16-Nov-2015 17:27 130k rem.txt 19-Oct-2015 17:50 151k .

... Parent Directory 05-Aug-2008 17:34 - 66ophN_1.eps 15-Apr-2008 13:18 187k 66ophN_2.eps 15-Apr-2008 13:18 188k 66ophN_3.eps 15-Apr-2008 13:18 193k 66ophN_4.eps 15-Apr-2008 13:18 182k 66ophN_5.eps 15-Apr-2008 13:18 147k 66ophS_art_1.eps 10-Jun-2009 05:08 91k 66ophS_art_2.eps 10-Jun-2009 05:08 97k 66ophS_art_3.eps 10-Jun-2009 05:08 97k 66ophS_art_4.eps 10-Jun-2009 05:09 100k 66ophS_art_5.eps 10-Jun-2009 05:09 102k 66ophS_art_6.eps ...

. Please standby and you will be automatically connected to the new location of the unframed Supernova page. Or, click on the link above. If you have questions or problems, please email me at David Bishop dbishop@vhdl.org . Last modified: Mon Aug 27 12:40:15 EDT 2001

... 2000 October 23 . Dwarf Elliptical Galaxy NGC 205 in the Local Group . ... It is part of a gathering of about 25 galaxies known as the Local Group . ... Pictured on the lower left is one of the many dwarf ellipticals : NGC 205 . ... The above image shows NGC 205 to be unusual for an elliptical galaxy in that it contains at least two dust clouds (at 1 and 4 o'clock - they are visible but hard to spot) and signs of recent star formation . ... About APOD | ...

... Тематические конференции: Общая астрономическая , Astro.com.ru , у "Звездочета" ; . ... Рейтинг страниц в теме: . Астрономические обсерватории (и их подразделения). ... Оценено и сдано в архив! . ... Laboratory of photographic astrometry of Pulcovo Observatory . ... Главная астрономическая обсерватория (Пулково) . ... Group of the Sun study (SAO) . ... Laboratory of radio-astronomical observations (SAO) . ... CODE laboratory (SAO) . ... НАЗАД, В СПИСОК КАТЕГОРИЙ (титульная страница AstroTop-100) . ...

... Here is a brief outline of the current theory of the events in the early history of the solar system: . A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own gravity. ... The gas cools off enough for the metal, rock and (far enough from the forming star) ice to condense out into tiny particles. (i.e. some of the gas turns back into dust). ... Once the larger of these particles get big enough to have a nontrivial gravity, their growth accelerates. ...