Seminar
Gas and Star Formation in Nearby Galaxies
Resumen
I will present results from the "Local Volume HI Survey'' (LVHIS), including a multi-wavelength atlas of 82 nearby galaxies. The LVHIS project targets all nearby, gas-rich galaxies with vLG < 550 km/s or D < 10 Mpc that are detected in the "HI Parkes All-Sky Survey" (HIPASS). A declination limit of DEC < -30 degrees was chosen for observations with the Australia Telescope Compact Array (ATCA). The majority of LVHIS galaxies are dwarf galaxies, but we also mapped the disks and outskirts of several very large galaxies (eg M83).
I will also introduce the Australian Square Kilometre Array Pathfinder (ASKAP) which consists of 36 x 12-m dishes, each equipped with Phased-Array Feeds, operating from 0.7 to 1.8 GHz. With a field-of-view of 30 square degr ASKAP is a fast 21-cm survey machine. Early Science with 12 antennas has started and I will present first results on our target field: nearby groups and clusters.
Sobre la charla
Australia Telescope National Facility, CSIRO, Australia
iCalendar I will also introduce the Australian Square Kilometre Array Pathfinder (ASKAP) which consists of 36 x 12-m dishes, each equipped with Phased-Array Feeds, operating from 0.7 to 1.8 GHz. With a field-of-view of 30 square degr ASKAP is a fast 21-cm survey machine. Early Science with 12 antennas has started and I will present first results on our target field: nearby groups and clusters.&location=&trp=false&ctz=Atlantic/Canary' target='_blank' rel='nofollow' class='btn btn-primary btn-sm text-light' title='Export to Google Calendar'> Google Calendar