{"id":55,"date":"2019-01-06T18:01:51","date_gmt":"2019-01-06T18:01:51","guid":{"rendered":"http:\/\/oliverpfuhl.com\/?page_id=55"},"modified":"2019-01-13T14:33:44","modified_gmt":"2019-01-13T14:33:44","slug":"science","status":"publish","type":"page","link":"https:\/\/oliverpfuhl.com\/?page_id=55","title":{"rendered":"Science"},"content":{"rendered":"\n<h2 class=\"wp-block-heading\">Highlights 2018<\/h2>\n\n\n\n<div class=\"wp-block-media-text alignwide\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"509\" src=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orbit-1024x509.png\" alt=\"\" class=\"wp-image-69\" srcset=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orbit-1024x509.png 1024w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orbit-300x149.png 300w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orbit-768x382.png 768w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orbit.png 1393w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-small-font-size wp-block-paragraph\"><strong><em><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2018\/10\/aa34294-18\/aa34294-18.html\">GRAVITY collaboration, et al. 2018b, Astronomy &amp; Astrophysics, 618, L10 <\/a><\/em><\/strong><br>We <strong>detected orbital motion at the innermost stable orbit of the supermassive black hole<\/strong> SgrA*. This discovery not only provides compelling evidence for a supermassive black hole but also has the potential to probe the spin in the near future. <br><br><a href=\"https:\/\/www.eso.org\/public\/news\/eso1835\/\">Link to ESO press release<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"983\" src=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orion-1024x983.png\" alt=\"\" class=\"wp-image-65\" srcset=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orion-1024x983.png 1024w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orion-300x288.png 300w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orion-768x737.png 768w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_orion.png 1056w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-small-font-size wp-block-paragraph\"><strong><em><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2018\/12\/aa33575-18\/aa33575-18.html\">GRAVITY collaboration: Karl, Pfuhl et al. 2018, Astronomy &amp; Astrophysics, 620, 116<\/a><\/em><\/strong><br><strong>High mass star formation<\/strong>. Several mechanisms have been proposed to explain the formation of massive stars in the face of radiation pressure.&nbsp; My master student and I observed in a recent study the Orion Nebulae, a proto-typical massive star formation region. We used interferometry to test formation models through the detection of gravitationally bound companion stars. Our results pose a challenge to current formation models based on the large number of detected low mass companions. <\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"390\" src=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/3C273-1024x390.png\" alt=\"\" class=\"wp-image-80\" srcset=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/3C273-1024x390.png 1024w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/3C273-300x114.png 300w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/3C273-768x293.png 768w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/3C273.png 1272w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-small-font-size wp-block-paragraph\"><br><strong><em><a href=\"https:\/\/www.nature.com\/articles\/s41586-018-0731-9?WT.feed_name=subjects_physics\">Sturm, Dexter, Pfuhl et al. 2018, Nature, 563, 657<\/a><\/em><\/strong><em><strong> <\/strong><\/em><strong>:<\/strong><br> We used <strong>spectro-astrometry with GRAVITY on the massive quasar 3C273<\/strong>, with the goal of measuring the <strong>broad-line region (BLR). <\/strong>This region, so far only accessible through indirect techniques, can be probed by an astrometric shift across the emission line. In this proto-typical system we were able to answer a long standing question on the orging of the BLR emission. We could show that the BLR is<strong> dominated by Keplerian rotation <\/strong>of high velocity clouds. Further, we obtained the black hole mass and BLR size with unprecedented accuracy. <br><br><a href=\"http:\/\/www.mpe.mpg.de\/6966658\/news20181129\">Link to MPE press release<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"312\" src=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_S2-1024x312.png\" alt=\"\" class=\"wp-image-71\" srcset=\"https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_S2-1024x312.png 1024w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_S2-300x91.png 300w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_S2-768x234.png 768w, https:\/\/oliverpfuhl.com\/wp-content\/uploads\/2019\/01\/Fig_S2.png 1522w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-small-font-size wp-block-paragraph\"><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2018\/07\/aa33718-18\/aa33718-18.html\"> <\/a><strong><em><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2018\/07\/aa33718-18\/aa33718-18.html\">GRAVITY collaboration, et al. 2018a, Astronomy &amp; Astrophysics, 615, L15<\/a><\/em><\/strong><br>We measured the <strong>general relativistic redshift<\/strong> of the star S2 as it passed the supermassive black hole SgrA* at a distance of only 17 light hours (GRAVITY collaboration, et al. 2018a). I played a key role especially in the <strong>astrometric analysis and orbit reconstruction<\/strong>. The immediate next objective of this project is the detection of Schwarzschild precession and higher order post-Newtonian perturbations of the S2 orbit. <br><br><a href=\"https:\/\/www.eso.org\/public\/news\/eso1825\/\">Link to ESO press release<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator\"\/>\n\n\n\n<!--nextpage-->\n\n\n\n<p class=\"wp-block-paragraph\">Older science highlights will be added soon&#8230;.<br><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Highlights 2018 GRAVITY collaboration, et al. 2018b, Astronomy &amp; Astrophysics, 618, L10 We detected orbital motion at the innermost stable orbit of the supermassive black hole SgrA*. This discovery not only provides compelling evidence for a supermassive black hole but also has the potential to probe the spin in the near future. Link to ESO [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-55","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/pages\/55","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=55"}],"version-history":[{"count":22,"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/pages\/55\/revisions"}],"predecessor-version":[{"id":217,"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=\/wp\/v2\/pages\/55\/revisions\/217"}],"wp:attachment":[{"href":"https:\/\/oliverpfuhl.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=55"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}