SpS5 - I. Obscured and distant clusters

Bibcode
2015HiA....16..410H
DOI
10.1017/S1743921314011776
Hanson, M. M.; Froebrich, D.; Martins, F.; Chené, A.-N.; Rosslowe, C.; Herrero, A.; Kim, H.-J.
Bibliographical reference

Highlights of Astronomy, Volume 16, pp. 410-419

Advertised on:
3
2015
Number of authors
7
IAC number of authors
1
Citations
0
Refereed citations
0
Description
This first part of Special Session 5 explored the current status of infrared-based observations of obscured and distant stellar clusters in the Milky Way galaxy. Recent infrared surveys, either serendipitously or using targeted searches, have uncovered a rich population of young and massive clusters. However, cluster characterization is more challenging as it must be obtained often entirely in the infrared due to high line-of-sight extinction. Despite this, much is to be gained through the identification and careful analysis of these clusters, as they allow for the early evolution of massive stars to be better constrained. Further, they act as beacons delineating the Milky Way's structure and as nearby, resolved analogues to the distant unresolved massive clusters studied in distant galaxies.
Type
Non-refereed
Galaxies
Luminosity function

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