Open AccessMulti‐epoch infrared photometric study of the star‐forming region G173.58+2.45
Author(s) -
Varricatt Watson P.,
Davis Christopher J.,
Adamson Andrew J.
Publication year - 2005
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2005.08882.x
Subject(s) - physics , astrophysics , outflow , astronomy , accretion (finance) , star formation , infrared , epoch (astronomy) , collimated light , stars , laser , meteorology , optics
We present a multi‐epoch infrared photometric study of the intermediate‐mass star‐forming region G173.58+2.45. Photometric observations are obtained using the near‐infrared JHKL ′ M ′ filters and narrow‐band filters centred at the wavelengths of the H 2 (1−0) S(1) (2.122 μm) and [Fe ii ] (1.644 μm) lines. The H 2 image shows molecular emission from shocked gas, implying the presence of multiple star formation and associated outflow activity. We see evidence for several collimated outflows. The most extended jet is at least 0.25 pc in length and has a collimation factor of ∼10, which may be associated with a binary system within the central cluster, resolved for the first time here. This outflow is found to be episodic, probably occurring or being enhanced during the periastron passage of the binary. We also find that the variable star in the vicinity of the outflow source, which was known as a FU Ori‐type star, is probably not a FU Ori object. It does, however, drive a spectacular outflow, and the variability is likely to be related to accretion, when large clouds of gas and dust spiral in towards the central source. Many other convincing accretion–outflow systems and YSO candidates are discovered in the field.