SUMMARY OF PROPOSAL 41013
GRADUATE YUICHI KAMATA
NAGOYA UNIVERSITY
AICHI JAPAN 464-01
NAGOYA-SHI
FURO-CHO, CHIKUSA-KU

  E-mail: KAMATA@SATIO.PHYS.NAGOYA-U.AC.JP	Tel: 81-52-789-2921	Fax: 81-52-789-2919
  Medium: 4GBDAT

Subject: STARS                                                       
  Title: NEARBY STAR FORMING REGION, LUPUS3                                              


Abstract:
 Lupus3 is the nearby(140pc) star forming region with a high star forming effciency
 of >6%. Half of the whole emission-line objects (T Tauri) in the lupus region(1-4)
 extending to 10deg are concentrated within this reion (1 square degree). Any of the
 IRAS point sources do not coincides with the soft X-ray sources observed by ROSAT
 PSPC, on the other hand, many emission-line objects coincide with the soft X-ray
 sources. This indicate that there exist many deeply embedded sources such as
 youngest protostars which are visible in the hard X-ray (>5keV) observation same as
 the case of the ASCA observation of Rho Ophiuchi dark cloud.

 Co-Is:
   1  AKIRA MIZUNO        	NAGOYA UNIVERSITY             JAPAN     
      (No Co-I contact data)
   2  KENGO TACHIHARA     	NAGOYA UNIVERSITY             JAPAN     
   3  YUZURU TAWARA       	NAGOYA UNIVERSITY             JAPAN     
   4  KAZUTOSHI HAGA      	NAGOYA UNIVERSITY             JAPAN     


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
LUPUS3                 1  242.2150  -39.1320    40   N   N   P  0.30000   1