Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
HIA / NRC
DRAO, Penticton, Canada
National Research Council, Herzberg Institute for Astrophysics, DRAO., Penticton, Canada
DRAO
Dominion Radio Astrophysical Observatory, Penticton, Canada
Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council, PO Box 248, Penicton, BC, Canada V2A 6K3
Dominion Radio Astrophysical Observatory, Penticton, British Columbia, Canada
Alberta, University, Edmonton, Canada
National Research Council Canada, Herzberg Institute of Astrophysics, Dominion Radio Astrophysical Observatory, Penticton, BC V2A 6J9, Canada
National Research Council of Canada
Dominion Astrophysical Observatory, Penticton, British Columbia, Canada
Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council, PO Box 248, Penticton, BC V2A 6K3, Canada
National Research Council of Canada, British Columbia, Canada
Dominion Radio Astrophysical Observatory, P.O. Box 248, Penticton, BC V2A 6K3, Canada
Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada, P.O. Box 248, Penticton, BC V2A 6J9, Canada
Dominion Radio Astrophysical Observatory, Penticton, BC, Canada
Herzberg Institute of Astrophysics, Penticton, Canada
HIA, National Research Council
DRAO, PO Box 248, Penticton, BC, V2A 6K3, Canada
HIA, Canada
National Research Council of Canada, Herzberg Institute of Astrophysics, Dominion Radio Astrophysical Observatory, Penticton, British Columbia V2A 6K3, Canada
National Research Council, Dominion Radio Astronomical Observatory, Penticton, BC, Canada
National Research Council Canada
Dominion Radio Astrophysical Observatory, Box 248, Penticton, British Columbia V2A 6K3, Canada
1420 and 408 MHz observations of the planetary nebulae BD + 30 deg 3639 and AFGL 618
A 408-MHz aperture synthesis radio telescope
A coherent lenticular Faraday rotation feature in the galactic interstellar medium.
A comparison of observations of H I dissociation zones with evolutionary models.
A cross-correlation receiver for radio astronomy employing quadrature channel generation by computed Hilbert transform
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Profile ID: LFWR-SCP-P-92617