... We have studied scaling relations (virial mass versus CO luminosity, luminosity versus size, linewidth versus size) for molecular clouds in the 30 Dor and N 159 regions in the Large Magellanic Cloud. ... The study of molecular clouds in the Galaxy has resulted in a number of scaling relations between global cloud properties such as mass, density, luminosity, size and velocity dispersion (e.g. Larson (1981) , Scoville & Sanders (1987) , Solomon et al. ... Elmegreen B.G., 1989, ApJ , 338 , 178. ...

ОТЧЕТ Об итогах голосования на внеочередном общем собрания акционеров открытого акционерного общества «Красногорский завод им. С.А. Зверева» (далее по тексту - «ОАО КМЗ, Общество»). ... Сокращенное фирменное наименование общества: ОАО КМЗ. ... Секретарь собрания - Секретарь совета директоров ОАО КМЗ Кожемякин Сергей Анатольевич. ... Число голосов, которыми обладали лица, включенные в список лиц, имевших право на участие в Собрании, не заинтересованные в совершении Обществом сделки - 2 218 926 голосов. ...

Supernova 1987A in LMC . One day in 1987, an astronomer by the name of Ian Shelton was making observations of the Tarantula Nebula in Large Magellanic cloud at Las Campanas Observatory, and he noticed something strange on his image. ... SN 1987A got as bright as 2.7, the only other recent SN even to come close was 1885A in M31 which got up to mag 6. ... Mag 4.5 . ... IAUC 4318 2/25/87 Type II? ... IAUC 7354 2/1/00 New structure in the inner ring . ... IAUC 7360 2/7/00 HST observation of new spot . ...

... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...

... LMC Project Outline . NGC 1818 Initial Results . ... The Large Magellanic Cloud (LMC) is uniquely suitable for the study of massive star clusters at all stages of evolution. By combining HST observations of these clusters with N-body models we hope to understand the origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond. ... We aim to combine our HST observations with N-body models to understand the formation and evolution of globular clusters. ...

Revolution: 2210 . POS_2210_120102_191_00_0002.XMM . ... 2012-01-02 | ... PSF version: 2210_06.PSF . ... Slew: 4260 secs . ... Obs_dur: 7382 secs . ... 001: 6229 sec . ... 002: 6234 sec . ... 003: 4884 sec . ... Obs_dur: 41000 secs . ... 004: 39986 sec . ... 005: 39981 sec . ... 001: 39847 sec . ... 002: 39852 sec . ... 006: 7868 sec . ... 16:55:02 ... exp continues . ... 003: 36207 sec . ... 007: 7868 sec . ... 008: 7868 sec . ... 009: 7868 sec . ... 010: 6438 sec . ... Slew: 5055 secs . ...

... Telescopes in the southern and northern hemispheres, with a longitude difference that enables students to observe the night sky in daytime classes, are linked by Internet2 to campuses in Louisville, Kentucky, and Toowoomba, Queensland. ... Kent Observatory in Australia offers the center of the Milky Way, the Magellanic Clouds, and transient events not visible from mid-latitudes in the northern hemisphere. ... The Observatories . ... Northern hemisphere: Moore Observatory near Louisville, Kentucky . ...

... GALAXY: A galaxy is made up of billions or trillions of stars bound together by their own gravity. ... HELIUM (He): The second element in the periodic table, has 2 protons, 2 neutrons, and is a noble gas. ... Helium melts at -272.2 degrees Celsius, and boils at -268.934 degrees Celsius. ... HYDROGEN (H): The first element on the periodic table, is a gas, and has an atomic mass of 1.00794 amu. ... Hydrogen melts at -259.34 degrees Celsius, and freezes at -252.87 degrees Celsius. ...