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Grain growth in the envelopes and disks of Class I protostars

Miotello, A. and Testi, L. and Lodato, G. and Ricci, L. and Rosotti, G. and Brooks, K. and Maury, A. and Natta, A. (2014) Grain growth in the envelopes and disks of Class I protostars. Astronomy and Astrophysics, 567 . Art. No. A32. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20141009-133535247

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Abstract

We present new 3 mm ATCA data of two Class I young stellar objects (YSOs) in the Ophiucus star forming region: Elias29 and WL12. For our analysis we compare them with archival 1.1 mm SMA data. In the (u,v) plane the two sources present a similar behavior: a nearly constant non-zero emission at long baselines, which suggests the presence of an unresolved component and an increase of the fluxes at short baselines, related to the presence of an extended envelope. Our data analysis leads to unusually low values of the spectral index α_(1.1−3 mm), which may indicate that mm-sized dust grains have already formed both in the envelopes and in the disk-like structures at such early stages. To explore the possible scenarios for the interpretation of the sources we perform a radiative transfer modeling using a Monte Carlo code, in order to take into account possible deviations from the Rayleigh-Jeans and optically thin regimes. Comparison between the model outputs and the observations indicates that dust grains may form aggregates up to millimeter size already in the inner regions of the envelopes of Class I YSOs. Moreover, we conclude that the embedded disk-like structures in our two Class I YSOs are probably very compact, in particular in the case of WL12, with outer radii down to tens of AU.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201322945 DOIArticle
http://arxiv.org/abs/1405.0821arXivDiscussion Paper
ORCID:
AuthorORCID
Testi, L.0000-0003-1859-3070
Additional Information:© 2014 ESO. Article published by EDP Sciences Received 30 October 2013; Accepted 1 May 2014; Published online 07 July 2014. The authors wish to thank ATNF & CSIRO staff for the support and the hospitality, F. Trotta and F. Testi for their help during the observing session. The authors also thank E. van Dishoeck and the referee, J. Jørgensen, for insightful comments that significantly improved our work. This work was partly supported by the ESO DGDF program and by the Italian Ministero dell’Istruzione, Università e Ricerca through the grant Progetti Premiali 2012-iALMA.
Funders:
Funding AgencyGrant Number
European Southern Observatory (ESO)UNSPECIFIED
Ministero dell'Istruzione, dell'Università e della Ricerca (MIUR)2012-iALMA
Subject Keywords:circumstellar matter; opacity; radiative transfer; protoplanetary disks; stars: protostars; dust, extinction
Record Number:CaltechAUTHORS:20141009-133535247
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141009-133535247
Official Citation:Grain growth in the envelopes and disks of Class I protostars A. Miotello, L. Testi, G. Lodato, L. Ricci, G. Rosotti, K. Brooks, A. Maury and A. Natta A&A 567 A32 (2014) DOI: http://dx.doi.org/10.1051/0004-6361/201322945
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:50314
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Oct 2014 20:50
Last Modified:22 Nov 2019 23:27

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