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The 4830 MHz Formaldehyde Line Observations of Dark Clouds in IC 1795 (W3)

  • Y. K. Minn (a1) and J. Mayo Greenberg (a2)

Abstract

A survey of H2CO absorption in dark clouds in IC 1795 (W3) shows that the material in the direction of W3 can be distinctly separated into three groups: one, immediately surrounding W3, has a uniform velocity of about −41 km–1 s; the second, associated with the W3 (OH) source has a velocity of about −49 km–1 s; the third, as a velocity of about −20 km–1 s and may be associated with an interarm spur in the foreground.

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Copyright

Corresponding author

* Present address: Dept. of Physics and Astronomy, University of Alabama.

References

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The 4830 MHz Formaldehyde Line Observations of Dark Clouds in IC 1795 (W3)

  • Y. K. Minn (a1) and J. Mayo Greenberg (a2)

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