Integral field spectroscopy of massive young stellar objects in the N113 H II region in the Large Magellanic Cloud

Ward, J.L.; Oliveira, J.M.; Van Loon, J. Th.; Sewiło, M.

Abstract

The Spitzer Surveying the Agents of Galaxy Evolution (SAGE) survey has allowed the identification and analysis of significant samples of Young Stellar Object (YSO) candidates in the Large Magellanic Cloud (LMC). However, the angular resolution of Spitzer is relatively poor meaning that at the distance of the LMC, it is likely that many of the Spitzer YSO candidates in fact contain multiple components. We present high-resolution K-band integral field spectroscopic observations of the three most prominent massive YSO candidates in the N113 H?II region using Very Large Telescope/Spectrograph for INtegral Field Observations in the Near Infrared (VLT/SINFONI). We have identified six K-band continuum sources within the three Spitzer sources and we have mapped the morphology and velocity fields of extended line emission around these sources. Br ?, He?I and H2 emission is found at the position of all six K-band sources; we discuss whether the emission is associated with the continuum sources or whether it is ambient emission. H2 emission appears to be mostly ambient emission and no evidence of CO emission arising in the discs of YSOs has been found. We have mapped the centroid velocities of extended Br ? emission and He?I emission and found evidence of two expanding compact H?II regions. One source shows compact and strong H2 emission suggestive of a molecular outflow. The diversity of spectroscopic properties observed is interpreted in the context of a range of evolutionary stages associated with massive star formation.

Citation

Ward, J., Oliveira, J., Van Loon, J. T., & Sewiło, M. (2016). Integral field spectroscopy of massive young stellar objects in the N113 H II region in the Large Magellanic Cloud. Monthly Notices of the Royal Astronomical Society, 455(3), 2345 - 2362. https://doi.org/10.1093/mnras/stv2424

• Journal Article Type: Article
• Acceptance Date: Oct 19, 2015
• Online Publication Date: Nov 21, 2015
• Publication Date: Jan 21, 2016
• Publicly Available Date: May 26, 2023
• Journal: Monthly Notices of the Royal Astronomical Society
• Print ISSN: 0035-8711
• Publisher: Oxford University Press
• Peer Reviewed: Peer Reviewed
• Volume: 455
• Issue: 3
• Pages: 2345 - 2362
• DOI: https://doi.org/10.1093/mnras/stv2424
• Keywords: circumstellar matter; stars: formation; stars: protostars; Magellanic Clouds; infrared stars
• Publisher URL: https://doi.org/10.1093/mnras/stv2424