TY - JOUR
T1 - PROTOSTELLAR OUTFLOWS in L1340
AU - Walawender, Josh
AU - Wolf-Chase, Grace
AU - Smutko, Michael
AU - Olinger-Luscusk, Joann
AU - Moriarty-Schieven, Gerald
N1 - Funding Information:
This work is based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, and France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This work is based on observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium. This publication makes use of data products from the Widefield Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of the VizieR catalog access tool, CDS, Strasbourg, France.
Publisher Copyright:
© 2016. The American Astronomical Society. All rights reserved.
PY - 2016/12/1
Y1 - 2016/12/1
N2 - We have searched the L1340 A, B, and C clouds for shocks from protostellar outflows using the H2 2.122 μm near-infrared line as a shock tracer. Substantial outflow activity has been found in each of the three regions of the cloud (L1340 A, L1340 B, and L1340 C). We find 42 distinct shock complexes (16 in L1340 A, 11 in L1340 B, and 15 in L1340 C). We were able to link 17 of those shock complexes into 12 distinct outflows and identify candidate source stars for each. We examine the properties (A V, T bol, and L bol) of the source protostars and compare them to the properties of the general population of Class 0/I and flat spectral energy distribution protostars and find that there is an indication, albeit at low statistical significance, that the outflow-driving protostars are drawn from a population with lower A V, higher L bol, and lower T bol than the general population of protostars.
AB - We have searched the L1340 A, B, and C clouds for shocks from protostellar outflows using the H2 2.122 μm near-infrared line as a shock tracer. Substantial outflow activity has been found in each of the three regions of the cloud (L1340 A, L1340 B, and L1340 C). We find 42 distinct shock complexes (16 in L1340 A, 11 in L1340 B, and 15 in L1340 C). We were able to link 17 of those shock complexes into 12 distinct outflows and identify candidate source stars for each. We examine the properties (A V, T bol, and L bol) of the source protostars and compare them to the properties of the general population of Class 0/I and flat spectral energy distribution protostars and find that there is an indication, albeit at low statistical significance, that the outflow-driving protostars are drawn from a population with lower A V, higher L bol, and lower T bol than the general population of protostars.
KW - HerbigHaro objects
KW - ISM: jets and outflows
KW - stars: formation
KW - stars: jets
KW - stars: pre-main sequence
KW - stars: protostars
UR - http://www.scopus.com/inward/record.url?scp=85004075863&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85004075863&partnerID=8YFLogxK
U2 - 10.3847/0004-637X/832/2/184
DO - 10.3847/0004-637X/832/2/184
M3 - Article
AN - SCOPUS:85004075863
SN - 0004-637X
VL - 832
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 184
ER -