Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-06-22T23:52:57.363Z Has data issue: false hasContentIssue false
  • English
  • Français

Hidden star clusters in the starburst galaxy He 2-10

Published online by Cambridge University Press:  26 May 2016

William D. Vacca ,
Kelsey E. Johnson  and
Peter S. Conti
William D. Vacca
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1312, D-85741 Garching-bei-München, BRD
Kelsey E. Johnson
Affiliation:
National Radio Astronomy Observatory, PO Box 0, Socorro, NM 87801, USA
Peter S. Conti
Affiliation:
Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, CO 80309-0440, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

N-band (10.8 μm) imaging of the blue compact starburst galaxy He 2-10 reveals the presence of four emission regions, which have no optical or near-IR counterparts. These sources correspond to the ‘ultradense H ii’ regions recently identified in 2cm and 6cm radio maps of this galaxy. We have used the N-band data to place constraints on the properties of the stellar clusters, that are deeply embedded within these dust-emitting regions.

Type
Part 3. Location and Distribution of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 574 - 575
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Kobulnicky, H.A., Johnson, K.E. 1999, ApJ 527, 154.Google Scholar
Meurer, G.R., Heckman, T.M., Leitherer, C., et al. 1995, AJ 110, 2665.Google Scholar
Vacca, W.D., Johnson, K.E., Conti, P.S. 2002, AJ 123, 772.Google Scholar