The Formaldehyde Masers in NGC 7538 and G29.96-0.02: VLBA, MERLIN, and VLA Observations

Abstract

The 6 cm formaldehyde (H2CO) maser sources in the compact HII regions NGC 7538-IRS1 and G29.96-0.02 have been imaged at high resolution (beams < 50 mas). Using the VLBA and MERLIN, we find the angular sizes of the NGC 7538 masers to be ~10 mas (30 AU) corresponding to brightness temperatures ~10^8 K. The angular sizes of the G29.96-0.02 masers are ~20 mas (130 AU) corresponding to brightness temperatures ~10^7 K. Using the VLA, we detect 2 cm formaldehyde absorption from the maser regions. We detect no emission in the 2 cm line, indicating the lack of a 2 cm maser and placing limits on the 6 cm excitation process. We find that both NGC 7538 maser components show an increase in intensity on 5-10 year timescales while the G29.96-0.02 masers show no variability over 2 years. A search for polarization provides 3-sigma upper limits of 1% circularly polarized and 10% linearly polarized emission in NGC 7538 and of 15% circularly polarized emission in G29.96-0.02. A pronounced velocity gradient of 28 km/s/arcsecond (1900 km/s/pc) is detected in the NGC 7538 maser gas.

accepted to ApJ, 15 figures, 11 tables

References in corpus (7)

• Does IRAS 16293-2422 have a hot core? Chemical inventory and abundance changes in its protostellar environment
• Non-Equilibrium Photodissociation Regions: Ionization-Dissociation Fronts
• Low Velocity Ionized Winds from Regions Around Young O Stars
• 5cm OH masers as diagnostics of physical conditions in star-forming regions
• A photoionization model of the compact HII region G29.96-0.02
• Submillimeter Imaging Polarimetry of the NGC 7538 Region
• Mid-Infrared Detection of a Hot Molecular Core in G29.96-0.02

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