Research Project
Grant-in-Aid for Scientific Research (C)
The ultimate goal of this project is to find out the origin of time variation of brightness of T Tauri stars by monitor observations at infrared wavelength. The origin is supposed to associate with the surface activities of T-Tauri star as well as activity at the contact region between the photosphere and the disk. Infrared monitor observations are still very limited in area as well as the time intervals.We prepared infrared camera and small telescope, which enable us to use rather wide field of view covering approximately 0.3 square degree of arc, to realize efficient observations. The system also has capability to observe several T Tauri stars as well as flux standard stars (second calibrators) in a single field of view. The sensitivities of the system, with 10 of signal-to-noise ratio at 20 minutes of exposure, are 17 magnitude at J band, 15.5 magnitude at H band, and 14 magnitude at K' band, whose depth is enough to observe T Tauri stars in Taurus star forming regions (lying at 140pc from us). To develop the camera part, we first started evaluation of InSb infrared array which is a test model of the infrared camera on board ASTRO-F mission. We carried out the evaluations using liquid He cooled chamber to operate the sensor device, COGITO-3 multi control system to operate the detector, and 32 cm Newtonian telescope in Komaba campus. The optics to minimize the Coma aberration was also developed to get a wide field of view at infrared wavelength. We have made monitor observations of T Tauri stars and been extending the projected observations of star forming regions with ASTRO-F.
All 2002 2001 2000 Other
All Journal Article (8 results) Publications (11 results)
The Astrophysical Journal 572
The Astrophysical Journal Vol.572
Pub.Astron.Soc.Japan 153
Pages: 2074-2088
Pub.Astron.Soc.Japan Vol.153
SPIE 4013
Pages: 114-122
Mid- and Far Infrared Astronomy and Future Space Missions ISAS research note Special issue 14
Pages: 19-26
120006837955
SPIE vol.4013
Mid-and Far Infrared Astronomy and Future Space Missions ISAS research note Special issue Vol.14