We present new Submillimeter Array and Plateau de Bure Interferometer observations of the intermediate-mass object IRAS 22198+6336 in the millimeter continuum and in several molecular line transitions. The millimeter continuum emission reveals a strong and compact source with a mass of ∼5M ⊙ and with properties of Class 0 objects. CO emission shows an outflow with a quadrupolar morphology centered on the position of the dust condensation. The CO outflow emission seems to come from two distinct outflows, one of them associated with SiO outflow emission. A large set of molecular lines has been detected toward a compact dense core clearly coincident with the compact millimeter source, and showing a velocity gradient perpendicular to the outflow traced by CO and SiO. The chemically rich spectrum and the rotational temperatures derived from CH3CN and CH3OH (100-150 K) indicate that IRAS 22198+6336 is harboring one of the few intermediate-mass hot cores known at present. © 2010 The American Astronomical Society. All rights reserved.
CITATION STYLE
Sánchez-Monge, Á., Palau, A., Estalella, R., Kurtz, S., Zhang, Q., Di Francesco, J., & Shepherd, D. (2010). IRAS 22198+6336: Discovery of an intermediate-mass hot core. Astrophysical Journal Letters, 721(2 PART 2). https://doi.org/10.1088/2041-8205/721/2/L107
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