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Rasseyannye zvezdnye skopleniya M35 i NGC 2158
3.01.2013 | Astronomicheskaya kartinka dnya
Rasseyannye skopleniya zvezd byvayut blizkimi i dalekimi, molodymi i starymi,
razrezhennymi i kompaktnymi.
Rasseyannye skopleniya
obychno soderzhat ot sta do desyati tysyach zvezd, sformirovavshihsya primerno v odno vremya.
V samyh molodyh rasseyannyh skopleniyah
obychno prisutstvuyut yarkie golubye zvezdy.
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