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ISO detection of CO+ toward the protostar IRAS 16293-2422

Rudolph, A.; Ceccarelli, C.; Caux, E.; Wolfire, M.; Nisini, B.; Saraceno, P. and White, G. J. (1997). ISO detection of CO+ toward the protostar IRAS 16293-2422. In: American Astronomical Society Meeting Abstract, 06-10 Jan 1998, Washington D.C., #121.04.

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We report the detection of eight high-N rotational transitions of CO+ towards a low mass protostar, IRAS 16293-2422. The source was observed with the Long Wavelength Spectrometer on board the Infrared Space Observatory. This is the first time that CO+ has been detected in a low luminosity source and the first time that high-N lines have been detected in any source. The detection of these lines is totally unpredicted by models and, consequently, their interpretation is a challenge. We discuss the possibility that the observed CO+ emission originates in the dense inner regions illuminated by the UV field created in the accretion shock (formed by the infalling material), and conclude that this is an improbable explanation. We have also considered the possibility that a strong, dissociative J-shock at ~ 500 AU from the star is the origin of the CO+ emission. This model predicts CO+ column densities in rough agreement with the observations if the magnetic field is ~ 1 mG and the shock velocity is 100 km s-1

Item Type: Conference or Workshop Item
Copyright Holders: 1997 AAS
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
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Item ID: 32684
Depositing User: G. J. White
Date Deposited: 21 Mar 2012 17:01
Last Modified: 07 Dec 2018 10:03
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