SUMMARY OF PROPOSAL 61026

MS YOHKO TSUBOI
TSUBOI@CR.SCPHYS.KYOTO-U.AC.JP

KYOTO UNIV.
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA-OIWAKE-CHO, SAKYO
Tel: 075-753-3843 Fax: 075-701-5377
Medium: 2.5GB8MM
Subject: STARS

DEEP SURVEY OF THE YOUNGEST PROTOSTARS IN OMC-2,3 CLOUD


ABSTRACT

In the Orion observation (PV phase), we detected faint sources in the OMC 2--3 region. These sources are well correspondent with filament structure of 1.3 mm continuum emission. This wave length traces the densest region (Av$>$100mag) in a cloud, the detected objects are coincident with 'the younger protostars', i.e., the early phase in Class I, and Class 0. Our proposal is TO OBSERVE THIS REGION DEEPLY (100 ksec) and our goal is TO CONFIRM THE DETECTION OF SUCH AN EXTREMELY YOUNG PROTOSTARS.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
KATSUJI KOYAMAKYOTO UNIV.JAPAN
MASAHIKO HAYASHINAOJAPAN
NAOTO KOBAYASHIHAWAII UNIV.JAPAN
SHIGEO YAMAUCHIIWATE UNIV.JAPAN
YUUTAROU SEKIMOTOUNIV. OF TOKYOJAPAN
KENNICHI TATEMATSUNAOJAPAN
TOMOFUMI UMEMOTONAOJAPAN
HANS ZINNECKERPOTSDAM INST.GERMANY
KENJI HAMAGUCHIKYOTO UNIV.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)OMC2-3
3
83.8658 -5.1021 40 ksN
Y
P
0.20000
1