Примеры использования Star formation на Английском языке и их переводы на Русский язык
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the study of comets and meteorites and star formation processes; the influence of microgravity on cell metabolism
the rate of star formation increases as some clouds meet the Jeans criterion, and collapse to form new stars. .
There is currently no star formation in CVn I and the measurements have so far failed to detect neutral hydrogen in it-the upper limit is 30,000 solar masses.
confirms the previous notion that old, foreground OB stars triggered star formation in this cloud.
This is because over the lifetime of the galaxy, star formation rates have been greater in the denser central regions,
demonstrate that star formation in dwarf galaxies does not occur continuously
Observations of globular clusters show that these stellar formations arise primarily in regions of efficient star formation, and where the interstellar medium is at a higher density than in normal star-forming regions.
instead contain a bright central structure with intense star formation that looks like a bulge when the galaxy is viewed face-on.
not enough on average for star formation, which indicates that local processes have a role.
Currently there is no star formation in Uma II.
This discovery points to a complicated star formation history of this galaxy.
Currently, there is no star formation in Segue 2.
This region of active current star formation is about 7000 light-years distant.
massive stars or shows traces of recent star formation.
Thus the formation of planetary systems is thought to be a natural result of star formation.
This star formation begins enshrouded in the collapsing cloud,
The galaxy contains stars of all ages, contains significant amounts of gas, and has experienced recent star formation.
Varying density in the N44 nebula has caused the formation of several dust pillars that may conceal star formation.
Even without circumstellar dust, regions undergoing star formation exhibit high infrared luminosities compared to stars on the main sequence.
C58 is notable for its very high rate of cooling which is unexplained by standard theories of neutron star formation.