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Chapter and Conference Paper
CO emission from the southern galactic plane and galactic structure
The original southern galactic plane CO survey (294° ⩽ 358° and 2° ⩽ ℓ ⩽ 13° at −0°.075 ⩽ b ⩽ 0°0.75) has been extended to cover the longitude range 279° ⩽ ℓ ⩽ 300° at −0°.95 ⩽ b ⩽ −0.70. The Carina arm is wel...
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Article
The Australian radio-telescope
A large synthesis radio telescope is under construction in Australia at a cost of $A 30.7million. In comprises a 6 km-long ‘compact array’ of 22 m antenna at Culgoora and a ‘long baseline array’ of 319 km, ach...
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Chapter
CO Observations, Geometry, and Galactic Structure
2.6 mm carbon monoxide and 21 cm hydrogen line observations of the Galaxy define six directions where gas is seen tangentially along a spiral feature and four directions where extended structures cross the R = R ...
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Chapter
The Australian Radio-Telescope
A large synthesis radio telescope is under construction in Australia at a cost of $A 30.7 million. In comprises a 6 km-long ‘compact array’ of 22 m antenna at Culgoora and a ‘long baseline array’ of 319 km, ac...
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Article
CO observations, geometry, and galactic structure
2.6 mm carbon monoxide and 21 cm hydrogen line observations of the Galaxy define six directions where gas is seen tangentially along a spiral feature and four directions where extended structures cross theR=R 0 c...