Paper:	Mapping Observation toward Protostellar Core L1527
Volume:	476, New Trends in Radio Astronomy in the ALMA Era
Page:	375
Authors:	Kiyokane, K.; Saito, M.; Saigo, K.; Kurono, Y.; Momose, M.; Tsukagoshi, T.; NRO45m SF-Legacy Team
Abstract:	We observed C18O(1-0) line emission toward a low-mass prtostellar core L1527 in the Taurus Molecular Cloud at a distance of 140 pc with the Nobeyama 45 m telescope to reveal the velocity structure closely related to the evolution of low-mass star forming cores. We obtained a wide map covering 6' × 6' ,∼0.2 pc × 0.2pc) with 15″ spatial resolution and with a noise level of ∼0.1 K in TA* with 0.1 km/s. We found an increase of the velocity dispersion toward the molecular outflow in the 2nd moment map. This may be related to the mechanism of dispersing the parent dense core.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.080 seconds