The Orion Fingers: H_2 Temperatures and Excitation in an Explosive Outflow
Abstract
We measure H_2 temperatures and column densities across the Orion Becklin-Neugebauer/Kleinmann-Low (BN/KL) explosive outflow from a set of 13 near-infrared (IR) H_2 rovibrational emission lines observed with the TripleSpec spectrograph on Apache Point Observatory's 3.5 m telescope. We find that most of the region is well characterized by a single temperature (~2000–2500 K), which may be influenced by the limited range of upper-energy levels (6000–20,000 K) probed by our data set. The H_2 column density maps indicate that warm H2 comprises 10^(-5)–10^(−3) of the total H_2 column density near the center of the outflow. Combining column density measurements for co-spatial H_2 and CO at T = 2500 K, we measure a CO/H2 fractional abundance of 2 × 10^(−3) and discuss possible reasons why this value is in excess of the canonical 10^(−4) value, including dust attenuation, incorrect assumptions on co-spatiality of the H_2 and CO emission, and chemical processing in an extreme environment. We model the radiative transfer of H_2 in this region with ultraviolet (UV) pumping models to look for signatures of H_2 fluorescence from H i Lyα pumping. Dissociative (J-type) shocks and nebular emission from the foreground Orion H ii region are considered as possible Lyα sources. From our radiative transfer models, we predict that signatures of Lyα pumping should be detectable in near-IR line ratios given a sufficiently strong source, but such a source is not present in the BN/KL outflow. The data are consistent with shocks as the H_2 heating source.
Additional Information
© 2018. The American Astronomical Society. Received 2018 January 31; revised 2018 March 3; accepted 2018 March 5; published 2018 April 6. We thank the referee for suggestions that improved the manuscript, and Jeremy Darling, Jason Glenn, Serena Criscuoli, and Mihály Horányi for thoughtful guidance on the methodology and analysis. Facility: Apache Point Observatory (TripleSpec). Software: Astropy (Robitaille et al. 2013), IPython (Perez & Granger 2007), Matplotlib (Hunter 2007), molecular-hydrogen (https://github.com/keflavich/molecular_hydrogen), NumPy and SciPy (van der Walt et al. 2011).Attached Files
Published - Youngblood_2018_ApJ_857_7.pdf
Files
Name | Size | Download all |
---|---|---|
md5:62c9c3de6093e7bedcfa86066e922548
|
3.7 MB | Preview Download |
Additional details
- Alternative title
- The Orion Fingers: H2 Temperatures and Excitation in an Explosive Outflow
- Eprint ID
- 85684
- Resolver ID
- CaltechAUTHORS:20180406-095409590
- Created
-
2018-04-09Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field