604 citations · 779 across the 14 of their papers we have counts for
14 papers
Kinematic clues to the origins of starless HI clouds : dark galaxies or tidal debris ?
R. Taylor, J. I. Davies, P. Jáchym +5
Isolated HI clouds with no optical counterparts are often taken as evidence for galaxy-galaxy interactions, though an alternative hypothesis is that these are primordial 'dark gala…
The Arecibo Galaxy Environment Survey IX: The Isolated Galaxy Sample
R. F. Minchin, R. Auld, J. I. Davies +6
We have used the Arecibo L-band Feed Array to map three regions, each of 5 square degrees, around the isolated galaxies NGC 1156, UGC 2082, and NGC 5523. In the vicinity of these g…
Can galaxy growth be sustained through HI-rich minor mergers?
M. D. Lehnert, W. van Driel, R. Minchin
Local galaxies with specific star-formation rates (star-formation rate per unit mass; sSFR~0.2-10/Gyr) as high as distant galaxies (z~1-3), are very rich in HI. Those with low stel…
SIGGMA: A Survey of Ionized Gas in the Galaxy, Made with the Arecibo Telescope
B. Liu, T. Mclntyre, Y. Terzian +5
A Survey of Ionized Gas in the Galaxy, made with the Arecibo telescope (SIGGMA) uses the Arecibo L-band Feed Array (ALFA) to fully sample the Galactic plane (30 < l < 75 and -2 < b…
Extragalactic HI Surveys at Arecibo: the Future
Riccardo Giovanelli
Starting in the 1970s, the Arecibo 305m telescope has made seminal contributions in the field of extragalactic spectroscopy. With the Gregorian upgrade completed in the late 1990s,…
Conference Summary: HI Science in the Next Decade
Martha P. Haynes
The atomic hydrogen (HI) 21cm line measures the gas content within and around galaxies, traces the dark matter potential and probes volumes and objects that other surveys do not. O…