CaltechAUTHORS
  A Caltech Library Service

An HST/STIS view of protoplanetary discs in Upper Scorpius: observations of three young M stars

Walker, Sam and Millar-Blanchaer, Maxwell Andrew and Ren, Bin and Kalas, Paul and Carpenter, John (2021) An HST/STIS view of protoplanetary discs in Upper Scorpius: observations of three young M stars. Monthly Notices of the Royal Astronomical Society, 504 (2). pp. 3074-3083. ISSN 0035-8711. doi:10.1093/mnras/stab1080. https://resolver.caltech.edu/CaltechAUTHORS:20210729-153815249

[img] PDF - Published Version
See Usage Policy.

8MB
[img] PDF - Accepted Version
See Usage Policy.

2MB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20210729-153815249

Abstract

We present observations of three protoplanetary discs in visible scattered light around M-type stars in the Upper Scorpius OB association using the Space Telescope Imaging Spectrograph (STIS) instrument on the Hubble Space Telescope (HST). The discs around stars 2MASS J16090075–1908526, 2MASS J16142029–1906481, and 2MASS J16123916–1859284 have all been previously detected with the Atacama Large Millimeter/submillimeter Array (ALMA), and 2MASS J16123916–1859284 has never previously been imaged at scattered light wavelengths. We process our images using reference star differential imaging, comparing and contrasting three reduction techniques – classical subtraction, Karhunen–Loève Image Projection, and non-negative matrix factorization, selecting the classical method as the most reliable of the three for our observations. Of the three discs, two are tentatively detected (2MASS J16142029–1906481 and 2MASS J16123916–1859284), with the third going undetected. Our two detections are shown to be consistent when varying the reference star or reduction method used, and both detections exhibit structure out to projected distances of ≳200 au. Structures at these distances from the host star have never been previously detected at any wavelength for either disc, illustrating the utility of visible-wavelength observations in probing the distribution of small dust grains at large angular separations.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stab1080DOIArticle
https://arxiv.org/abs/2104.06447arXivDiscussion Paper
ORCID:
AuthorORCID
Walker, Sam0000-0001-7062-815X
Millar-Blanchaer, Maxwell Andrew0000-0001-6205-9233
Ren, Bin0000-0003-1698-9696
Kalas, Paul0000-0002-6221-5360
Carpenter, John0000-0003-2251-0602
Additional Information:© 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2021 April 13. Received 2021 April 8; in original form 2020 December 11. Published: 17 April 2021. We thank John H. Debes for providing the algorithmic mask in Debes et al. (2017). This research has made extensive use of NUMPY (Harris et al. 2020), SCIPY (Virtanen et al. 2020), and MATPLOTLIB (Hunter 2007). The results of this paper are based on observations made with the NASA/ESA Hubble Space Telescope. We thank support from GO 15176 and GO 15497 provided by NASA through a grant from STScI under NASA contract NAS 5-26555. JC acknowledges support from the National Aeronautics and Space Administration under grant no. 15XRP15_20140 issued through the Exoplanets Research Program. Data Availability: The data underlying this paper are available in their raw form via the HST MAST archive under programs GO 15176 and GO 15497. Processed data are available from the author on request.
Funders:
Funding AgencyGrant Number
NASANAS 5-26555
NASA15XRP15_20140
Issue or Number:2
DOI:10.1093/mnras/stab1080
Record Number:CaltechAUTHORS:20210729-153815249
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210729-153815249
Official Citation:Sam Walker, Maxwell Andrew Millar-Blanchaer, Bin Ren, Paul Kalas, John Carpenter, An HST/STIS view of protoplanetary discs in Upper Scorpius: observations of three young M stars, Monthly Notices of the Royal Astronomical Society, Volume 504, Issue 2, June 2021, Pages 3074–3083, https://doi.org/10.1093/mnras/stab1080
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:110063
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Aug 2021 19:03
Last Modified:02 Aug 2021 19:03

Repository Staff Only: item control page