<<

Nordic-Baltic Summer School Tuorla 8 - 18 June 2009

Properties of

Lecture 1

Bo Reipurth University of Hawaii WARNING/DISCLAIMER

This lecturer is seriously jet-lagged. His utterances are likely to contain much nonsense The Formation Newsletter

Abstracts Dissertation abstracts Meetings Jobs New Books Announcements

If you want to be notified by email when an issue has appeared, send your name and email address to [email protected]

http://www.ifa.hawaii.edu/users/reipurth/newsletter.htm PPV

University of Arizona Press 2007

Comprehensive reviews of star and formation HANDBOOK OF STAR FORMING REGIONS Astronomical Society of the Pacific, 2009 - 2000 pages - 105 authors 60 star forming regions within 2 kpc The Birth of Stars and

John Bally & Bo Reipurth

Cambridge University Press, 2007

Detection of Hα emission stars using objective prism

Reipurth et al. 2004

Infrared colors of Hα stars in NGC 2264 from 2MASS

Reipurth et al. 2004 Relation between Hα emission and IR excess

Carpenter et al. 2001 Periodic variability of young stars in

Doppler images of the V410 Tau at four different phases. The dark spots are regions that are cooler than the surrounding by at least 500 K. Herbst et al. 2000 VYSOS

A 20 inch telescope in Hawaii, and a 16 inch telescope in Chile, that monitor all star forming regions along the Galactic Plane. The field of view is 30 x 30 arcmin, with 0.45 arcsec pixels.

Proplyds in Orion

Basic concept of magnetospheric in T Tauri stars

Camenzind 1990

Reipurth, Pedrosa, Lago 1996

X-Z slice through the middle of the funnel stream at = 15°. The contour lines show the plane cross section of the density distribution inside the funnel stream. The density changes exponentially from = 0.2 (blue) to = 2.0 (red).

Red lines with arrows show selected magnetic field lines. The axis, Ω, and the magnetic moment, μ, are shown.

Romanova et al. 2004 Simulations by Marina Romanova The gas in the funnel flows crashes into the stellar photosphere and deposits in the upper layers. Variations in the infall leads to variability in the hot spot, and changes in the veiling The hot spot changes as the infalling gas moves around Variability of Funnel Flows

Frame rotating with star From some lines-of-sight the funnels can completely obscure the star Lamm et al. 2005