{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,10,4]],"date-time":"2026-10-04T11:18:28Z","timestamp":1791112708951,"version":"4.1.0"},"reference-count":40,"publisher":"American Association for the Advancement of Science (AAAS)","issue":"6143","content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Science"],"published-print":{"date-parts":[[2013,7,19]]},"abstract":"<jats:title>Accretion Analog<\/jats:title>\n          <jats:p>\n            Mass flow from a circumstellar disk onto a young star's surface plays an important role in the final stages of star formation but the details of this complex process are not well understood.\n            <jats:bold>\n              Reale\n              <jats:italic>et al.<\/jats:italic>\n            <\/jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" ext-link-type=\"doi\" issue=\"6143\" page=\"251\" related-article-type=\"in-this-issue\" vol=\"341\" xlink:href=\"10.1126\/science.1235692\">251<\/jats:related-article>\n            , published online 20 June) analyzed a solar flare that led to bright impacts of plasma onto the solar surface. Numerical simulations suggest that these events can be seen as analogs to accretion of matter onto stars and can thus be used to understand stellar accretion.\n          <\/jats:p>","DOI":"10.1126\/science.1235692","type":"journal-article","created":{"date-parts":[[2013,6,21]],"date-time":"2013-06-21T04:39:30Z","timestamp":1371789570000},"page":"251-253","source":"Crossref","is-referenced-by-count":52,"title":["Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: A Template for Stellar Accretion"],"prefix":"10.1126","volume":"341","author":[{"given":"Fabio","family":"Reale","sequence":"first","affiliation":[{"name":"Dipartimento di Fisica e Chimica, Universit\u00e0 di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy."},{"name":"Istituto Nazionale di Astrofisica (INAF)\/Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Salvatore","family":"Orlando","sequence":"additional","affiliation":[{"name":"Istituto Nazionale di Astrofisica (INAF)\/Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Paola","family":"Testa","sequence":"additional","affiliation":[{"name":"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 58, Cambridge, MA 02138, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Giovanni","family":"Peres","sequence":"additional","affiliation":[{"name":"Dipartimento di Fisica e Chimica, Universit\u00e0 di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy."},{"name":"Istituto Nazionale di Astrofisica (INAF)\/Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Enrico","family":"Landi","sequence":"additional","affiliation":[{"name":"Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]},{"given":"Carolus J.","family":"Schrijver","sequence":"additional","affiliation":[{"name":"Lockheed Martin Advanced Technology Center, Palo Alto, CA 94304, USA."}],"role":[{"vocabulary":"crossref","role":"author"}]}],"member":"221","reference":[{"key":"e_1_3_2_2_2","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/168.3.603"},{"key":"e_1_3_2_3_2","unstructured":"L. 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