
TY  - JOUR
A1  - Tovmassian, HM 
A1  - Shahbazian, ET 
T1  - Hydrogen Content of Young Stellar Clusters. II. Clusters NGC2175, 2264, 2353, and 2362
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1973
VL  - 26
IS  - 6
SP  - 837
EP  - 842
KW  - 
UR  - https://doi.org/10.1071/PH730837 
N2  - Measurements of the total amount of gaseous hydrogen associated with the O-type stellar clusters NGC 2175, 2264, 2353, and 2362 are reported. For the nebula in which NGC2175 is embedded, a mean electron density of 20cm- 3 and a mass of ionized hydrogen of 1400Mo were obtained. For the nebula in which NGC2264 is embedded, a mean electron density of 10 cm - 3 and a mass of ionized hydrogen of 60Mo (with a possible, though unlikely, additional 40Mo of neutral hydrogen) were obtained. No hydrogen in association with NGC 2353 or 2362 was detected. 
ER  -

