Water deuterium fractionation in the inner regions of two solar type protostars
Vianney Taquet, Ana L\`opez-Sepulcre, Cecilia Ceccarelli, Roberto, Neri, Claudine Kahane, Audrey Coutens, Charlotte Vastel

TL;DR
This study measures the water deuterium fractionation in two solar-type protostars, revealing similar chemical histories and providing insights into water formation in early stellar environments.
Contribution
First interferometric measurements of HDO/H2O ratios in IRAS2A and IRAS4A, expanding understanding of water chemistry in protostars.
Findings
Water deuterium fractionation is lower than that of formaldehyde and methanol.
Fractionation ratios are similar to IRAS16293-2422.
Protostars share a similar chemical history despite different locations.
Abstract
The [HDO]/[H2O] ratio is a crucial parameter for probing the history of water formation. So far, it has been measured for only three solar type protostars and yielded different results, possibly pointing to a substantially different history in their formation. In the present work, we report new interferometric observations of the HDO 4 2,2 - 4 2,3 line for two solar type protostars, IRAS2A and IRAS4A, located in the NGC1333 region. In both sources, the detected HDO emission originates from a central compact unresolved region. Comparison with previously published interferometric observations of the H218_2O line emissions, combined with published observations, provides a [HDO]/[H2O] ratio of 0.3 - 8 % in IRAS2A and 0.5 - 3 % in IRAS4A. First, the water…
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