The Ionized Circumstellar Envelopes of Orion Source I and the Becklin Neugebauer Object

Abstract

The 229 GHz (lambda 1.3mm) radio emission from Orion-KL was mapped with up to 0.14" angular resolution with CARMA, allowing measurements of the flux densities of Source I ('SrcI') and the Becklin-Neugebauer Object (BN), the 2 most massive stars in this region. We find integrated flux densities of 310 +/- 45 mJy for SrcI and 240 +/- 35 mJy for BN. SrcI is optically thick even at 229 GHz. No trace of the H30alpha recombination line is seen in its spectrum, although the v_2=1, 5(5,0)-6(4,3) transition of H2O, 3450 K above the ground state, is prominent. SrcI is elongated at position angle 140 degrees, as in 43 GHz images. These results are most easily reconciled with models in which the radio emission from SrcI arises via the H- free-free opacity in a T < 4500 K disk, as considered by Reid et al. (2007). By contrast, the radio spectrum of BN is consistent with p+/e- free-free emission from a dense (n_e ~ 5x10^7 cm^{-3}), but otherwise conventional, hypercompact HII region. The source is becoming optically thin at 229 GHz, and the H30alpha recombination line, at VLSR = 23.2 +/- 0.5 km/sec, is prominent in its spectrum. A Lyman continuum flux of 5x10^{45} photons/sec, consistent with that expected from a B star, is required to maintain the ionization. Supplementary 90 GHz observations were made to measure the H41alpha and H42alpha recombination lines toward BN. Published 43 and 86 GHz data suggest that SrcI brightened with respect to BN over the 15 year period from 1994 to 2009.

8 pages, 5 figures; accepted for publication in ApJ

References in corpus (7)

• The distance to the Orion Nebula
• Monitoring the Large Proper Motions of Radio Sources in the Orion BN/KL Region
• Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA
• Imaging the Ionized Disk of the High-Mass Protostar Orion-I
• A 1.3 cm wavelength radio flare from a deeply embedded source in the Orion BN/KL region
• The first detection of the 232 GHz vibrationally excited H2O maser in Orion KL with ALMA
• ALMA and VLA observations of recombination lines and continuum toward the Becklin-Neugebauer object in Orion

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