Chemical inventory of the envelope of the Class I protostar L1551 IRS 5
P. Marchand,
A. Coutens,
J. Scigliuto
et al.
Abstract:Episodic accretion in protostars leads to luminosity outbursts that end up heating their surroundings. This rise in temperature pushes the snow lines back, enabling the desorption of chemical species from dust grain surfaces, which may significantly alter the chemical history of the accreting envelope. However, a limited number of extensive chemical surveys of eruptive young stars have been performed thus far.
In the present study, we carry out a large spectral survey of the binary Class I protostar L1551 IRS… Show more
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