Home
Scholarly Works
Star Clusters in the Magellanic Type Irr Galaxy...
Journal article

Star Clusters in the Magellanic Type Irr Galaxy NGC 4449

Abstract

We compare the luminosity function of star clusters in the LMC and NGC 4449: a IBm/Sm type galaxy very similar in appearance and luminosity (MB = −18.5) to the LMC (MB = −18.4). The brightest of several hundred clusters in NGC 4449 have MV = −10 (assuming a distance of 3.9 Mpc), comparable to the brightest clusters in the LMC.

Authors

Seitzer P; Grebel E

Journal

Symposium - International Astronomical Union, Vol. 190, , pp. 468–469

Publication Date

January 1, 1999

DOI

10.1017/s0074180900118753

ISSN

0074-1809
View published work (Non-McMaster Users)

Contact the Experts team