{"id":1250,"date":"2021-04-15T16:36:19","date_gmt":"2021-04-15T15:36:19","guid":{"rendered":"https:\/\/sites.dundee.ac.uk\/stellarnursery?post_type=papers&#038;p=1250"},"modified":"2021-04-15T16:36:19","modified_gmt":"2021-04-15T15:36:19","slug":"a-rosetta-stone-for-protoplanetary-disks-the-synergy-of-multi-wavelength-observations","status":"publish","type":"papers","link":"https:\/\/sites.dundee.ac.uk\/stellarnursery\/papers\/a-rosetta-stone-for-protoplanetary-disks-the-synergy-of-multi-wavelength-observations\/","title":{"rendered":"A `Rosetta Stone&#8217; for Protoplanetary Disks: The Synergy of Multi-Wavelength Observations"},"content":{"rendered":"<div id=\"authors-and-aff\" class=\"s-authors-and-aff\">\n<ul class=\"list-inline\">\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Sicilia-Aguilar%2C+A.%22&amp;sort=date%20desc,%20bibcode%20desc\">Sicilia-Aguilar, A.<\/a><span class=\"affiliation\">\u00a0(<i>SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, KY16 9SS, St Andrews, UK<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Banzatti%2C+A.%22&amp;sort=date%20desc,%20bibcode%20desc\">Banzatti, A.<\/a><span class=\"affiliation\">\u00a0(<i>Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Carmona%2C+A.%22&amp;sort=date%20desc,%20bibcode%20desc\">Carmona, A.<\/a><span class=\"affiliation\">\u00a0(<i>Universit\u00e9 de Toulouse, UPS-OMP, IRAP, 14 avenue E. Belin, Toulouse, F-31400, France<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Stolker%2C+T.%22&amp;sort=date%20desc,%20bibcode%20desc\">Stolker, T.<\/a><span class=\"affiliation\">\u00a0(<i>Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Kama%2C+M.%22&amp;sort=date%20desc,%20bibcode%20desc\">Kama, M.<\/a><span class=\"affiliation\">\u00a0(<i>Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Mendigut%C3%ADa%2C+I.%22&amp;sort=date%20desc,%20bibcode%20desc\">Mendigut\u00eda, I.<\/a><span class=\"affiliation\">\u00a0(<i>School of Physics and Astronomy, University of Leeds, Woodhouse Lane, Leeds, LS2 9JT, UK<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Garufi%2C+A.%22&amp;sort=date%20desc,%20bibcode%20desc\">Garufi, A.<\/a><span class=\"affiliation\">\u00a0(<i>Universidad Auton\u00f3noma de Madrid, Dpto. F\u00edsica Te\u00f3rica, M\u00f3dulo 15, Facultad de Ciencias, Campus de Cantoblanco, E-28049 Madrid, Spain<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Flaherty%2C+K.%22&amp;sort=date%20desc,%20bibcode%20desc\">Flaherty, K.<\/a><span class=\"affiliation\">\u00a0(<i>Van Vleck Observatory, Astronomy Department, Wesleyan University, 96 Foss Hill Drive, Middletown, CT 06459<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22van+der+Marel%2C+N.%22&amp;sort=date%20desc,%20bibcode%20desc\">van der Marel, N.<\/a><span class=\"affiliation\">\u00a0(<i>Institute for Astronomy, University of Hawaii, Honolulu, 2680 Woodlawn Drive, Honolulu, HI 96822-1839, USA<\/i>)<\/span>;<\/li>\n<li class=\"author\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/#search\/q=author:%22Greaves%2C+J.%22&amp;sort=date%20desc,%20bibcode%20desc\">Greaves, J.<\/a><span class=\"affiliation\">\u00a0(<i>School of Physics &amp; Astronomy, Cardiff University, 4 The Parade, Cardiff CF24 3AA, UK<\/i>)<\/span><\/li>\n<\/ul>\n<\/div>\n<div class=\"s-abstract-text\">\n<h4 class=\"sr-only\">Abstract<\/h4>\n<p>Recent progress in telescope development has brought us different ways to observe protoplanetary disks: interferometers, space missions, adaptive optics, polarimetry, and time- and spectrally-resolved data. While the new facilities have changed the way we can tackle open problems in disk structure and evolution, there is a substantial lack of interconnection between different observing communities. Here, we explore the complementarity of some of the state-of-the-art observing techniques, and how they can be brought together to understand disk dispersal and planet formation.<\/p>\n<\/div>\n<p>&nbsp;<\/p>\n<dl class=\"s-abstract-dl-horizontal\">\n<dt>Publication:<\/dt>\n<dd>\n<div id=\"article-publication\">Publications of the Astronomical Society of Australia, Volume 33, id.e059\u00a031\u00a0pp.<\/div>\n<\/dd>\n<dt>Pub Date:<\/dt>\n<dd>December 2016<\/dd>\n<dt>DOI:<\/dt>\n<dd><a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2016PASA...33...59S\/doi:10.1017\/pasa.2016.56\" target=\"_blank\" rel=\"noreferrer noopener\" data-target=\"DOI\">10.1017\/pasa.2016.56<\/a>\u00a0<i class=\"fa fa-external-link\" aria-hidden=\"true\"><\/i><\/dd>\n<dt>arXiv:<\/dt>\n<dd><a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2016PASA...33...59S\/arxiv:1611.01798\" target=\"_blank\" rel=\"noreferrer noopener\" data-target=\"arXiv\">arXiv:1611.01798<\/a>\u00a0<i class=\"fa fa-external-link\" aria-hidden=\"true\"><\/i><\/dd>\n<dt>Bibcode:<\/dt>\n<dd><a href=\"https:\/\/ui.adsabs.harvard.edu\/#abs\/2016PASA...33...59S\/abstract\">2016PASA&#8230;33&#8230;59S\u00a0<\/a><i class=\"icon-help\" title=\"\" aria-hidden=\"true\" data-toggle=\"popover\" data-container=\"body\" data-content=\"The bibcode is assigned by the ADS as a unique identifier for the paper.\" data-original-title=\"\"><\/i><\/dd>\n<dt>Keywords:<\/dt>\n<dd>\n<ul class=\"list-inline\">\n<li>Astronomical instrumentation;<\/li>\n<li>methods and techniques;<\/li>\n<li>methods: observational;<\/li>\n<li>stars: formation;<\/li>\n<li>protoplanetary disks;<\/li>\n<li>Astrophysics &#8211; Solar and Stellar Astrophysics;<\/li>\n<li>Astrophysics &#8211; Earth and Planetary Astrophysics<\/li>\n<\/ul>\n<\/dd>\n<dt>E-Print Comments:<\/dt>\n<dd>Accepted for publication in PASA. 37 pages, 9 figures, 1 table. Revised version: corrected problem in Fig 2; doi:10.1017\/pasa.2016.56<\/dd>\n<\/dl>\n","protected":false},"featured_media":1251,"template":"","class_list":["post-1250","papers","type-papers","status-publish","has-post-thumbnail","hentry"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.7 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>A `Rosetta Stone&#039; for Protoplanetary Disks: The Synergy of Multi-Wavelength Observations - The Stellar Nursery<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/sites.dundee.ac.uk\/stellarnurserypapers\/a-rosetta-stone-for-protoplanetary-disks-the-synergy-of-multi-wavelength-observations\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"A `Rosetta Stone&#039; for Protoplanetary Disks: The Synergy of Multi-Wavelength Observations - The Stellar Nursery\" \/>\n<meta property=\"og:description\" content=\"Sicilia-Aguilar, A.\u00a0(SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, KY16 9SS, St Andrews, UK); Banzatti, A.\u00a0(Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA); Carmona, A.\u00a0(Universit\u00e9 de Toulouse, UPS-OMP, IRAP, 14 avenue E. 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