New stellar associations in M33 galaxy

Details New stellar associations in M33 galaxy New stellar associations in M33 galaxy

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.106..371k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 106, no. 2, Nov. 1984, p. 371-379.

Astronomy and Astrophysics

Astrophysics

15

Galactic Structure, Spiral Galaxies, Star Distribution, Astronomical Photometry, Galactic Nuclei, H Ii Regions, Stellar Evolution

Scientific paper

The greater part of the associations presently identified in the M 33 galaxy by comparing U and B system plates, extending the Humphreys and Sandage (1980) numeration, are located in the spiral arms. It is noted that another large part of the associations identified are connected with H II regions, and that young associations prevail in proximity to the nucleus. The associations outline two strong and two faint spiral arms that are as much as 4 kpc from the nucleus, and the farthest associations imply a diameter of 20 kpc.

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