{"id":42,"date":"2017-08-21T10:35:26","date_gmt":"2017-08-21T10:35:26","guid":{"rendered":"https:\/\/escience.aip.de\/iau30-fm4\/?page_id=42"},"modified":"2018-08-01T01:15:00","modified_gmt":"2018-08-01T01:15:00","slug":"programme","status":"publish","type":"page","link":"https:\/\/escience.aip.de\/iau30-fm4\/programme\/","title":{"rendered":"Programme"},"content":{"rendered":"

Invited talks are 25 min + 5 min
\nContributed talks are 15 min + 5 min<\/p>\n

August 30, 2018:<\/h1>\n

MAGNETIC FIELDS IN CORES AND FILAMENTS<\/h4>\n

8:30-9:00<\/strong>
\nJ. Soler: Review on Observations of magnetic fields in star-forming clouds
\n9:00-9:30<\/strong>
\nS. Inutsuka: Review on the role of magnetic field in the formation and evolution of filamentary molecular clouds
\n9:30-9:50<\/strong>
\nB.-G. Andersson: Interstellar Dust Grain Alignment
\n9:50-10:00<\/strong>
\nDiscussion<\/p>\n

13:30-13:50<\/strong>
\nJ. Kwon: Magnetic field structures in star-forming regions revealed by imaging polarimetry at multi-wavelengths
\n13:50-14:10<\/strong>
\nL. Fissel: The Formation of Dense Gas within Magnetized Molecular Clouds: A BLASTPol Study of the Vela C Giant Molecular Cloud
\n14:10-14:30<\/strong>
\nM. Tahani: Helical Magnetic Fields in Molecular Clouds? A New Method to Determine the Line-of-Sight Magnetic Field Structure in Molecular Clouds<\/p>\n

MAGNETIC FIELDS IN PROTOSTARS<\/h4>\n

14:30-15:00<\/strong>
\nP. Hennebelle: Theoretical review on the roles of magnetic fields during the main accretion phase<\/p>\n

15:15-16:15<\/strong>
\nPoster session<\/p>\n

August 31st, 2018:<\/h1>\n

MAGNETIC FIELDS IN PROTOSTARS (cont.)<\/h4>\n

08:30-09:00<\/strong>
\nS. Lai: Review on observations of magnetic fields during the main accretion phase
\n09:00-09:20<\/strong>
\nM. Galametz: The role of magnetic fields in the early stages of star formation – confronting observations with theoretical expectations
\n09:20-09:40<\/strong>
\nQ. Zhang: Magnetic fields and massive star formation
\n09:40-10:00<\/strong>
\nI. Stephens: Trying to Make Sense of Polarization Patterns in Circumstellar Disks<\/p>\n

10:30-10:50<\/strong>
\nD. Dall’Olio: Revealing magnetic fields towards massive protostars: a multi-scale approach using masers and dust
\n10:50-11:10<\/strong>
\nY. Tsukamoto: The impact of non-ideal effects on the circumstellar disk evolution and their observational signatures<\/p>\n

MAGNETIC FIELDS IN PMS STARS<\/h4>\n

11:10-11:40<\/strong>
\nM. Sch\u00f6ller: Observational review of magnetic fields in Herbig Ae\/Be stars
\n11:40-12:00<\/strong>
\nS. J\u00e4rvinen: Magnetic fields along the pre-main sequence: new magnetic field measurements of Herbig Ae stars using high resolution HARPS spectropolarimetry<\/p>\n

13:30-14:00<\/strong>
\nJ.-F. Donati: Review on observations of magnetic fields of T Tauri stars and their inner accretion discs
\n14:00-14:30<\/strong>
\nS. Lizano: Review on magnetized models of Protoplanetary Disks
\n14:30-14:50<\/strong>
\nA. Kospal: Magnetic field and accretion in the young eruptive star EX Lupi
\n14:50-15:00<\/strong>
\nDiscussion<\/p>\n

15:30-15:50<\/strong>
\nM. Flock: Magnetized disk models of young circumstellar disks
\n15:50-17:00<\/strong>
\nDiscussion<\/p>\n","protected":false},"excerpt":{"rendered":"

Invited talks are 25 min + 5 min Contributed talks are 15 min + 5 min August 30, 2018: MAGNETIC FIELDS IN CORES AND FILAMENTS 8:30-9:00 J. Soler: Review on Observations of magnetic fields in star-forming clouds 9:00-9:30 S. Inutsuka: Review on the role of magnetic field in the formation and evolution of filamentary molecular … Continue reading “Programme”<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/pages\/42"}],"collection":[{"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/comments?post=42"}],"version-history":[{"count":8,"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/pages\/42\/revisions"}],"predecessor-version":[{"id":138,"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/pages\/42\/revisions\/138"}],"wp:attachment":[{"href":"https:\/\/escience.aip.de\/iau30-fm4\/wp-json\/wp\/v2\/media?parent=42"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}