User Tools

Site Tools


usic:chara_array_chara

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Next revision Both sides next revision
usic:chara_array_chara [2019/07/10 18:44]
gail_stargazer
usic:chara_array_chara [2019/07/10 18:46]
gail_stargazer
Line 5: Line 5:
 ====== Center for High Angular Resolution Astronomy (CHARA) ====== ====== Center for High Angular Resolution Astronomy (CHARA) ======
  
-[[http://www.chara.gsu.edu/|The CHARA Array]] has conducted science observations since 2004.  The observing program now includes community access time through the NOAO peer review system.  As of July 2019, there are 184 refereed publications based on data from the CHARA Array.  Recent science results and investigations currently underway include:+[[http://www.chara.gsu.edu/|The CHARA Array]] has conducted science observations since 2004. The observing program now includes community access time through the NOAO peer review system. As of July 2019, there are 184 refereed publications based on data from the CHARA Array. Recent science results and investigations currently underway include:
  
   * Gravity darkening and oblateness of rapidly rotating main sequence stars.   * Gravity darkening and oblateness of rapidly rotating main sequence stars.
Line 15: Line 15:
   * Images of interacting binaries.   * Images of interacting binaries.
   * Images of a binary star system in eclipse.   * Images of a binary star system in eclipse.
-  * Precision masses in spatially resolved spectroscopic binaries.+  * Precision stellar masses of spatially resolved spectroscopic binaries.
   * Direct detection of high contrast companions around Cepheids, RS CVn, and Be stars.   * Direct detection of high contrast companions around Cepheids, RS CVn, and Be stars.
   * Structure and physical properties of circumstellar disks around Be stars.   * Structure and physical properties of circumstellar disks around Be stars.
   * Images of disks and winds around young stellar objects.   * Images of disks and winds around young stellar objects.
-  * Earliest measurements of the angular expansion of a nova after an eruption.+  * Early measurements of the angular expansion of a nova after an eruption.
   * Direct images of starspots.   * Direct images of starspots.
   * Images of convection cells on supergiant stars.   * Images of convection cells on supergiant stars.
usic/chara_array_chara.txt ยท Last modified: 2019/07/10 18:51 by gail_stargazer