Herbig–Haro Outflows in Circinus W
Creators
- 1. Department of Physics and Astronomy, University of Alaska Anchorage, Anchorage, AK 99508 (United States)
- 2. Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001 (United States)
- 3. The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)
Description
We report the discovery of new Herbig–Haro (HH) outflows in the Western Circinus molecular cloud. They were found using a color-composite imaging method that reveals faint Hα emission in complex environments. Follow-up observations in [S ii] confirmed their classification as HH objects. Nearly half of the newly discovered objects are part of the HH 76 outflow and are associated with a likely young stellar object (YSO) candidate. We also identify the source of a second outflow. Three newly discovered objects are part of a third outflow whose origin is unknown. Four more HH objects are also discovered, each of which has a location and morphology that does not suggest an origin. In total there must be at least five YSOs in the field currently producing outflows. The discovery of new HH objects and associated driving sources in this cloud complex provides more evidence for active star formation and a relatively young age in this seldom-studied region.
Availability note (English)
Available from http://dx.doi.org/10.3847/1538-3881/abb3d3Additional details
Identifiers
Publishing Information
- Journal Title
- Astronomical Journal (New York, N.Y. Online)
- Journal Volume
- 160
- Journal Issue
- 4
- Journal Page Range
- [8 p.]
- ISSN
- 1538-3881
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52053728
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; EMISSION; GALAXIES; HYDROGEN; STAR EVOLUTION
- Descriptors DEC
- ELEMENTS; EVOLUTION; NONMETALS