... December 30, 1995 . LMC X-1: A Black Hole Candidate . ... Explanation: The strongest source of X-rays in the Large Magellanic Cloud originates from an unusually energetic binary star system . This strong source, dubbed LMC X-1, is thought to be a normal and compact star orbiting each other. ... Motion in the binary system indicates the compact star is probably a black hole , since its high mass - roughly five times that of our Sun - should be enough to cause even a neutron star to implode. ...

... Sternberg Astronomical Institute , Moscow University . ... Present edition unites two parts of Catalogue of interacting galaxies by B.A.Vorontsov-Velyaminov: the first part (Part 1) containing 355 systems was published in 1959 [1] and the second one (Part 2) with 497 objects - in 1976 [2].Thus two published parts of Catalogue include 852 interacting systems. ... All new of them (1162 by number) were taken from the comments to the galaxies in Morphological catalogue by Vorontsov-Velyaminov et al.[ ...

... 2000 September 21 . XZ Tauri System Ejects Gas Bubble . ... Explanation: Why is the binary star system XZ Tauri emitting a hot bubble of expanding gas? ... The XZ Tauri star system is known to reside in the Taurus star forming region located about 500 light-years away. ... The bubble has been expanding over the past thirty years and now extends to nearly fifteen times the binary separation. Tomorrow's picture: Star Cluster . ... About APOD | ...

... 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. ...

. This is the faintest SNe, at mag. 18.3, yet detected by my system. Mike Schwartz , Director . Tenagra Observatories, Ltd. Cottage Grove, OR 97424 . Back to Bright Supernovae . David Bishop Last modified: Tue Feb 16 08:42:58 EST 1999

New GCVS Version (GCVS5) FileName Explanations ----------------------------------------------------------------- ReadMe This file GCVS5 The ... ------------------------------------------------------ 1- 2 I2 --- Constell [1/88]Constellation numeric code 3- 6 I4 --- Number Star number within the constellation 7 A1 --- Component *Component identification 9- 18 A10 --- GCVS * Variable ... Field is non-blank if magMin is a magnitude or amplitude given in a system other than that indicated by magCode. ...

... Астрономические данные в Сети - где искать и как пользоваться? Сайты с астрономической библиографией . ... Солнечные сайты . ... Астероидные сайты . ... http://www.uic.rsu.ru/astro/ А наиболее полный список на сайты по теме " что почитать по астрономии " (по-русски) можно найти в соответствующем разделе рейтингового каталога АстроТоп-100 . ... Прекрасная система поиска позволит Вам найти обзорные статьи практически по любому разделу современной науки - от физики и астрономии до химии и биологии. ...

... The distance scales of the objects are matched both by comparing the first derivatives of the angular velocity determined separately from radial velocities and proper motions and by the statistical-parallax method. ... Good agreement between the inferred 0 and our calculations based on space velocities suggests that the Lindblad relation holds throughout the entire sample volume. ... Brandt and Blitz (1993) published the distances and radial velocities for a total of 206 H II-regions. ... Astron. ...