{"id":20442,"date":"2018-01-04T13:27:30","date_gmt":"2018-01-04T12:27:30","guid":{"rendered":"http:\/\/www.h-its.org\/?p=20442"},"modified":"2019-03-22T10:00:46","modified_gmt":"2019-03-22T09:00:46","slug":"califa_en","status":"publish","type":"post","link":"https:\/\/www.h-its.org\/de\/2018\/01\/04\/califa_en\/","title":{"rendered":"Library of galaxy histories reconstructed from motions of stars"},"content":{"rendered":"\n<figure class=\"wp-block-image\"><a class=\"dt-single-image\" href=\"http:\/\/www.h-its.org\/wp-content\/uploads\/2018\/01\/starproj_sample_rotated.png\"><img decoding=\"async\" src=\"http:\/\/www.h-its.org\/wp-content\/uploads\/2018\/01\/starproj_sample_rotated-300x300.png\" alt=\"\" class=\"wp-image-20438\" \/><\/a><figcaption> A simulated galaxy from the Auriga project used to test the modelling method applied to CALIFA galaxies. (image: Robert Grand, HITS)[<\/figcaption><\/figure>\n\n\n\n<p><strong>The CALIFA survey allows to map the orbits of the stars of a sample of 300 galaxies, a fundamental information to know how they formed and evolved.&nbsp; HITS astrophysicists have collaborated in this project that was led by the Instituto de Astrof\u00edsica de Andaluc\u00eda, Spain. The results have been published in &#8222;Nature Astronomy.&#8220;<br><\/strong><\/p>\n\n\n\n<p><a href=\"http:\/\/www.iaa.es\/en\/news\/library-galaxy-histories-reconstructed-motions-stars\" target=\"_blank\" rel=\"noopener\"><em>See also the press release from the Instituto de Astrof\u00edsica de Andaluc\u00eda (IAA-CSIC), Spain<\/em><\/a><\/p>\n\n\n\n<p>Just like the Sun is moving in our galaxy, the Milky Way, all the stars in galaxies are moving, but with very different orbits: some of the stars have strong rotations, while others may be moving randomly with no clear rotation. Comparing the fraction of stars on different orbits we can find out how galaxies form and evolve. An international team of astronomers, among them <a href=\"http:\/\/www.h-its.org\/en\/research\/tap\/people\/\">Dandan Xu and Robert Grand from the Theoretical Astrophysics&nbsp; group (TAP)<\/a> at HITS, has derived directly, for the first time, the orbital distribution of a galaxy sample, containing more than 300 galaxies of the local universe. AmonThe results, <a href=\"https:\/\/www.nature.com\/articles\/s41550-017-0348-1\" target=\"_blank\" rel=\"noopener\">published in Nature Astronomy<\/a>, are based on the CALIFA survey, a project developed at Calar Alto Observatory and conceived from the Institute of Astrophysics of Andalusia (IAA-CSIC).<\/p>\n\n\n\n<p>Galaxies are the largest structures in the universe, and scientist study how they evolve to understand the history of the universe. Galaxy formation entails the hierarchical assembly of halos of dark matter (a type of matter that has not been directly observed and whose existence and properties are inferred from its gravitational effects), along with the condensation of normal matter at the halos\u2019 center, where stellar formation takes place. Stars that formed from a settled, thin gas disk and then lived though dynamically quiescent times will present near circular orbits, while stars with random motions are the result of turbulent environments, either at birth or later, with galactic mergers.<\/p>\n\n\n\n<p>Thus, the motions of stars in a galaxy are like a history book; they record the information about their birth and growth environment, and it may tell us how the galaxy was formed. \u201cHowever, the motion of each single star is not directly observable in external galaxies. External galaxies are projected on the observational plane as an image and we cannot resolve the discrete stars in it,\u201d says Ling Zhu, researcher from the Max Planck Institute for Astronomy who leads the study. \u201cThe CALIFA survey uses a recently developed technique, integral field spectroscopy, which can observe the external galaxies in such a way that it provides the overall motion of stars. Thus, we can get kinematic maps of each galaxy.\u201d<\/p>\n\n\n\n<p>The researchers then build models for each galaxy by superposing stars on different types of orbits. By constraining the model with the observed image and kinematic maps, they can find out the amount of stars moving on different types of orbits in each galaxy. They call it the stellar orbit distribution and, for this study, the team has built models for all 300 galaxies, representative of the general properties of galaxies in the local universe.<\/p>\n\n\n\n<p>The maps show changes in galactic orbit distribution depending on the total stellar mass of the galaxies. The ordered-rotating orbits are most prominent in galaxies with total stellar masses of 10 billion solar masses, and least important for the most massive ones. Random-motion orbits unsurprisingly dominate the most massive galaxies (more than 100 billion solar masses). \u201cThis is the first orbit-based mass sequence across all morphological types. It includes flourishing information of a galaxy\u2019s past, basically whether it had been a quiet succession of only smaller mergers or shaped by a violent major merger. Further studies are needed to understand the details,\u201d says Glenn van de Ven (ESO).<\/p>\n\n\n\n<p>The researchers had found a new and accurate method of reading off a galaxy\u2019s history &#8212; and their survey with its data sets for 300 galaxies turned out to be the largest existing library of galaxy history books.<\/p>\n\n\n\n<p>\u201cThis work highlights the importance of integral field spectroscopy and, in particular, of large-scale surveys such as the CALIFA project. The significant contribution of what we call \u2018hot\u2019 orbits, a mixture of rotation and random movements of the stellar component, poses important challenges to cosmological models of galaxy formation and evolution,\u201d says Rub\u00e9n Garc\u00eda Benito, a researcher at the Institute of Astrophysics of Andalusia (IAA-CSIC) participating in the project.<\/p>\n\n\n\n<p>CALIFA\u2019s results represent an observationally-determined orbit distribution of galaxies in the present-day universe. They lend themselves thus to direct comparison with samples of cosmological simulations of galaxies in a cosmological context. In this sense, these results open a new window for comparing galaxy simulations to the observed galaxy population in the present-day universe.<br><strong><em><a href=\"https:\/\/www.youtube.com\/watch?time_continue=29&amp;v=w67yS68qwto\" target=\"_blank\" rel=\"noopener\">See the CALIFA Youtube video<\/a>&nbsp;<\/em> <\/strong><\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Contact:<\/h2>\n\n\n\n<p>Silbia L\u00f3pez de Lacalle<br>Instituto de Astrof\u00edsica de Andaluc\u00eda (IAA-CSIC)<br>+34 958 230 676<br><a href=\"mailto:silbialo@iaa.es\">silbialo@iaa.es<\/a><\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Reference:<\/h2>\n\n\n\n<p>\u201cThe Stellar Orbit Distribution in Present-Day Galaxies Inferred from the CALIFA Survey,\u201d Ling Zhu et al., 2018 Jan. 1, Nature Astronomy [<a href=\"https:\/\/doi.org\/10.1038\/s41550-017-0348-1\">https:\/\/doi.org\/10.1038\/s41550-017-0348-1<\/a>, preprint: <a href=\"https:\/\/arxiv.org\/abs\/1711.06728\">https:\/\/arxiv.org\/abs\/1711.06728<\/a>].<\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Authors:<\/h2>\n\n\n\n<p>Ling Zhu, Glenn van de Ven, Remco van den Bosch, Hans-Walter Rix, Mariya Lyubenova, Jes\u00fas Falc\u00f3n-Barroso, Marie Martig, Shude Mao, DanDan Xu, Yunpeng Jin, Aura Obreja, Robert J. J. Grand, Aaron A. Dutton, Andrea V. Maccio, Facundo A. G\u00f3mez, Jakob C. Walcher, Rub\u00e9n Garc\u00eda-Benito, Stefano Zibetti, Sebastian F. S\u00e1nchez.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The CALIFA survey allows to map the orbits of the stars of a sample of 300 galaxies, a fundamental information to know &#8230;<\/p>\n","protected":false},"author":58,"featured_media":30143,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":""},"categories":[92,1329],"hits-research-group":[],"class_list":["post-20442","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-wissenschaftsnews","category-pressemitteilungen"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Library of galaxy histories reconstructed from motions of stars - HITS gGmbH<\/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:\/\/www.h-its.org\/de\/2018\/01\/04\/califa_en\/\" \/>\n<meta property=\"og:locale\" content=\"de_DE\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Library of galaxy histories reconstructed from motions of stars - 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