Star Formation Across the W3 Complex
- Author(s)
- Carlos G. Román-Zúñiga, Jason E. Ybarra, Guillermo D. Megías, Mauricio Tapia, Elizabeth A. Lada, Joáo F. Alves
- Abstract
We present a multi-wavelength analysis of the history of star formation
in the W3 complex. Using deep, near-infrared ground-based images
combined with images obtained with Spitzer and Chandra observatories, we
identified and classified young embedded sources. We identified the
principal clusters in the complex and determined their structure and
extension. We constructed extinction-limited samples for five principal
clusters and constructed K-band luminosity functions that we compare
with those of artificial clusters with varying ages. This analysis
provided mean ages and possible age spreads for the clusters. We found
that IC 1795, the centermost cluster of the complex, still hosts a large
fraction of young sources with circumstellar disks. This indicates that
star formation was active in IC 1795 as recently as 2 Myr ago,
simultaneous to the star-forming activity in the flanking embedded
clusters, W3-Main and W3(OH). A comparison with carbon monoxide emission
maps indicates strong velocity gradients in the gas clumps hosting
W3-Main and W3(OH) and shows small receding clumps of gas at IC 1795,
suggestive of rapid gas removal (faster than the T Tauri timescale) in
the cluster-forming regions. We discuss one possible scenario for the
progression of cluster formation in the W3 complex. We propose that
early processes of gas collapse in the main structure of the complex
could have defined the progression of cluster formation across the
complex with relatively small age differences from one group to another.
However, triggering effects could act as catalysts for enhanced
efficiency of formation at a local level, in agreement with previous
studies.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Universidad Nacional Autonoma de Mexico, Universidad de Sevilla, University of Florida, Gainesville
- Journal
- The Astronomical Journal
- Volume
- 150
- No. of pages
- 18
- Publication date
- 09-2015
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Keywords
- ASJC Scopus subject areas
- Astronomy and Astrophysics, Space and Planetary Science
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/f739a5ce-23a1-41d7-88b7-7fc891295cb8