{"id":418,"date":"2021-02-03T05:52:02","date_gmt":"2021-02-03T05:52:02","guid":{"rendered":"https:\/\/sites.dundee.ac.uk\/stellarnursery?p=418"},"modified":"2021-04-15T19:32:44","modified_gmt":"2021-04-15T18:32:44","slug":"starmeltnews","status":"publish","type":"post","link":"https:\/\/sites.dundee.ac.uk\/stellarnursery\/news\/starmeltnews\/","title":{"rendered":"STAR-MELT"},"content":{"rendered":"<h1><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\"><b>STAR-MELT <\/b>(<strong>ST<\/strong>ellar <strong>A<\/strong>cc<strong>R<\/strong>etion &#8211; <strong>M<\/strong>apping with <strong>E<\/strong>mission <strong>L<\/strong>ine <strong>T<\/strong>omography)<\/span><\/span><\/h1>\n<p><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">An automated, portable and user-friendly <\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">Jupyter<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0notebook\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">created\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">to\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">analy<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">s<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">e time<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">-resolved<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0spectra of young stars.\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">By analy<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">s<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">ing the time- and velocity-signatures of the emission line spectra, STAR-MELT investigates the physical conditions (temperatures, densities), spatial location, and variability, of the line-emitting regions<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">. These<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0are typically well<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0beyond the limits of direct resolution and interferometry<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">, and include accretion channels, hot spots on and near the stellar surface, stellar and inner disk winds, and the innermost regions of protoplanetary disks.\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun ContextualSpellingAndGrammarErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">The\u00a0 code<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0is at this point available via collaboration\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">(please contact us if you are interested in using STAR-MELT) and\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">can already analyse data from the VLT spectroscopes (UVES, ESPRESSO, X-SHOOTER), plus FEROS, HARPS,\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">ESP<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">a<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">DO<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">n<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SpellingErrorV2 SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">S<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">, SOPHIE,<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">\u00a0<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">CHIRON, and can be easily converted to any facility that provides 1D wavelength-calibrated spectra<\/span><\/span><span class=\"TextRun SCXW254467096 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW254467096 BCX0\" data-ccp-parastyle=\"Body Text\">.<\/span><\/span><\/p>\n<h1>See Introduction Video to STAR-MELT below:<\/h1>\n<p><iframe title=\"STAR-MELT in 1 minute\" width=\"800\" height=\"450\" src=\"https:\/\/www.youtube.com\/embed\/grDMizYmU6U?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture\" allowfullscreen><\/iframe><\/p>\n<h1><span class=\"TextRun SCXW40122949 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW40122949 BCX0\"><strong>STAR-MELT<\/strong> has now been presented in several\u00a0<\/span><\/span><span class=\"TextRun SCXW40122949 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW40122949 BCX0\">international<\/span><\/span><span class=\"TextRun SCXW40122949 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW40122949 BCX0\">\u00a0<\/span><\/span><span class=\"TextRun SCXW40122949 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW40122949 BCX0\">conferences<\/span><\/span><span class=\"TextRun SCXW40122949 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW40122949 BCX0\">:\u00a0<\/span><\/span><\/h1>\n<h2><span class=\"TextRun MacChromeBold SCXW259089169 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW259089169 BCX0\" data-ccp-parastyle=\"heading 3\">Five years since HL Tau: A New Era in Planet Formation<\/span><\/span><\/h2>\n<p>Virtual Conference hosted by the European Space Agency, 7-11 December 2020<\/p>\n<p><a href=\"https:\/\/www.eso.org\/sci\/meetings\/2020\/hltau2020.html\" target=\"_blank\" rel=\"noopener\">Link to Conference Website<\/a><\/p>\n<p><a href=\"https:\/\/sites.dundee.ac.uk\/stellarnurseryresearch\/star-melt-python-package-talk-astronomical-emission-line-analysis\/\">Presentation by Justyn Campbell-White <\/a>\u00a0&#8211; <em>STAR-MELT Python Package Talk. Astronomical Emission Line Analysis<\/em><\/p>\n<p><a href=\"https:\/\/sites.dundee.ac.uk\/stellarnurseryresearch\/reading-between-the-lines-presentation-by-aurora-sicilia-aguilar\/\">Presentation by Aurora Sicilia-Aguilar<\/a> &#8211; <em>Reading between the lines Time-resolved adventures mapping young and wild stars<\/em><\/p>\n<h2><span class=\"TextRun MacChromeBold SCXW134566628 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW134566628 BCX0\" data-ccp-parastyle=\"heading 3\">Cool Stars 20.5<\/span><\/span><\/h2>\n<p>Virtual Conference hosted by Center for Astrophysics Harvard &amp; Smithsonian and Mit Kavli Institute\u00a0 March 2-4 2021<\/p>\n<p><a href=\"http:\/\/coolstars20.cfa.harvard.edu\/cs20half\/index.html\">Link to Conference Website<\/a><\/p>\n<p><a href=\"https:\/\/sites.dundee.ac.uk\/stellarnurseryresearch\/reading-between-the-lines-how-time-and-velocity-resolved-data-can-help-us-to-map-the-tiniest-scales-in-young-forming-stars\/\"><span class=\"TextRun BCX0 SCXW123526683\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun BCX0 SCXW123526683\" data-ccp-parastyle=\"Body Text\">Poster by Aurora Sicilia-Aguilar<\/span><\/span><\/a>\u00a0 &#8211; <em>\u201cReading Between the Lines\u201d: How Time &#8211; and Velocity-Resolved Data Can Help us to Map the Tiniest Scales in Young Forming Stars<\/em><\/p>\n<p><a href=\"https:\/\/sites.dundee.ac.uk\/stellarnurseryresearch\/introducing-star-melt-stellar-accretion-mapping-with-emission-line-tomography-a-python-package-for-extraction-identification-fitting-and-analysis-of-spectral-lines\/\">Poster and Video by Justyn Campbell-White<\/a> &#8211; <em>Introducing STAR-MELT: STellar AccRetion Mapping with Emission Line Tomography \u2013 A Python Package for Extraction, Identification, Fitting and Analysis of Spectral Lines<\/em><\/p>\n<p>&nbsp;<\/p>\n<h6><span class=\"TextRun MacChromeBold SCXW259089169 BCX0\" lang=\"EN-GB\" xml:lang=\"EN-GB\" data-contrast=\"auto\"><span class=\"NormalTextRun SCXW259089169 BCX0\" data-ccp-parastyle=\"heading 3\">\u00a0<\/span><\/span><\/h6>\n","protected":false},"excerpt":{"rendered":"<p>STAR-MELT (STellar AccRetion &#8211; Mapping with Emission Line Tomography) An automated, portable and user-friendly Jupyter\u00a0notebook\u00a0created\u00a0to\u00a0analyse time-resolved\u00a0spectra of young stars.\u00a0By analysing the time- and velocity-signatures of the emission line spectra, STAR-MELT investigates the physical conditions (temperatures, densities), spatial location, and variability, of the line-emitting regions. These\u00a0are typically well\u00a0beyond the limits of direct resolution and interferometry, and [&hellip;]<\/p>\n","protected":false},"author":11,"featured_media":1261,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[1],"tags":[],"class_list":["post-418","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.7 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>STAR-MELT - 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\/stellarnurserynews\/starmeltnews\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"STAR-MELT - The Stellar Nursery\" \/>\n<meta property=\"og:description\" content=\"STAR-MELT (STellar AccRetion &#8211; Mapping with Emission Line Tomography) An automated, portable and user-friendly Jupyter\u00a0notebook\u00a0created\u00a0to\u00a0analyse time-resolved\u00a0spectra of young stars.\u00a0By analysing the time- and velocity-signatures of the emission line spectra, STAR-MELT investigates the physical conditions (temperatures, densities), spatial location, and variability, of the line-emitting regions. 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