Skip to main content

High resolution observations of disks around protostellar sources with the Nobeyama Millimeter Array

  • Part I: Disks—Observation
  • Conference paper
  • First Online:
  • 137 Accesses

Part of the book series: Lecture Notes in Physics ((LNP,volume 465))

Abstract

We present high spatial resolution observations of disks around young stellar objects in Taurus with the Nobeyama Millimeter Array. A survey of circumstellar disks at 3 mm shows that the 3 mm continuum emission tends to be weaker for embedded sources than for visible T Tauri stars, which is consistent with our previous interpretation of protoplanetary disk formation. The CS gas around L1489 and IRAS 04365+2535 show disk-like structures of ∼1000 AU in radius. A 13CO observation of HL Tau indicates direct evidence of dynamical infalling motion. We discuss the formation of a centrifugally supported viscous accretion disk around HL Tau.

This is a preview of subscription content, log in via an institution.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Steven Beckwith Jakob Staude Axel Quetz Antonella Natta

Rights and permissions

Reprints and permissions

Copyright information

© 1996 Springer-Verlag

About this paper

Cite this paper

Ohashi, N., Hayashi, M. (1996). High resolution observations of disks around protostellar sources with the Nobeyama Millimeter Array. In: Beckwith, S., Staude, J., Quetz, A., Natta, A. (eds) Disks and Outflows Around Young Stars. Lecture Notes in Physics, vol 465. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0102626

Download citation

  • DOI: https://doi.org/10.1007/BFb0102626

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-61389-3

  • Online ISBN: 978-3-540-68511-1

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics