Dynamical estimates of gas - star complex total masses

Details Dynamical estimates of gas - star complex total masses Dynamical estimates of gas - star complex total masses

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26at....7..113d&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 7, Issue 2, pp.113-116

Astronomy and Astrophysics

Astronomy

1

Open Clusters, Tidal Effects, Gas-Star Complexes

Scientific paper

Gas-star complexes introduced by Efremov and Sitnik (1988) are approximated by ellipsoids. The total mass and the mean density of some complexes are estimated from the data on young open cluster sizes and their tidal sizes in the Galaxy gravitational field. The total mass ranges from 0.19 to 120 million solar masses, and the mean density ranges from 0.35 to 3.8 solar masses per cubic parsec.

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