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Stellar Associations in the Tail of NGC 4038

Published online by Cambridge University Press:  26 May 2016

I. Saviane ,
J. E. Hibbard  and
R. M. Rich
I. Saviane
Affiliation:
ESO, 3107 Alonso de Cordova, Vitacura - Casilla 19001, Santiago 19, Chile
J. E. Hibbard
Affiliation:
NRAO, 520 Edgemont Road, Charlottesville, VA 22903, USA
R. M. Rich
Affiliation:
Department of Physics & Astronomy, UCLA, Math-Sciences 8979, Los Angeles, CA 90095-1562, USA

Abstract

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We have used the Hubble Space Telescope and Wide Field Planetary Camera 2 to image the putative tidal dwarf galaxy located at the tip of the Southern tidal tail of NGC 4038/9, the Antennae. We resolve individual stars, and identify two stellar populations. Hundreds of massive stars are present, concentrated into tight OB associations on scales of 200 pc, with ages ranging from 2-100 Myr. An older stellar population is distributed roughly following the outer contours of the neutral hydrogen in the tidal tail; we associate these stars with material ejected from the outer disks of the two spirals. The older stellar population has a red giant branch tip at I = 26.5 ± 0.2 from which we derive a distance modulus (m - M)0 = 30.7 ± 0.25. The implied distance of 13.8 ± 1.7 Mpc is nearly a factor of two closer than commonly quoted distances for NGC 4038/9. In contrast to the previously studied core of the merger, we find no super star clusters. One might conclude that SSCs require the higher pressures found in the central regions in order to form, while spontaneous star formation in the tail produces the kind of O-B star associations seen in dwarf irregular galaxies.

Type
Part 4. Recycling
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 546 - 549
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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