BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Australia Telescope National Facility - ECPv6.16.1//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Australia Telescope National Facility
X-ORIGINAL-URL:https://www.atnf.csiro.au
X-WR-CALDESC:Events for Australia Telescope National Facility
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Australia/Sydney
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20240406T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20241005T160000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20250405T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20251004T160000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+1100
TZOFFSETTO:+1000
TZNAME:AEST
DTSTART:20260404T160000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+1000
TZOFFSETTO:+1100
TZNAME:AEDT
DTSTART:20261003T160000
END:DAYLIGHT
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20250219T150000
DTEND;TZID=Australia/Sydney:20250219T160000
DTSTAMP:20260514T003532
CREATED:20250217T115308Z
LAST-MODIFIED:20250217T115918Z
UID:13270-1739977200-1739980800@www.atnf.csiro.au
SUMMARY:Barbara Mazzilli Ciraulo's Colloquium
DESCRIPTION:Overview\n\nWinds and fountains in GECKOS star-forming galaxies \n\nDescribe the details of your eGalactic winds play a crucial role in galaxy evolution by expelling gas from the disk\, thereby limiting the fuel available for star formation. Simulations suggest these winds are the most important regulators of galaxy growth\, yet their mass outflow rates and phase distribution remain poorly constrained due to a lack of multi-phase observations spanning warm ionised\, cold molecular\, and atomic gas phases.I will present results from the GECKOS survey\, which combines deep VLT/MUSE observations with ALMA\, ASKAP-WALLABY and MeerKAT observations\, and upcoming JWST data to study galactic winds in edge-on galaxies. We resolve filamentary outflows from star-forming knots in the disk at ~100 pc scales. By quantifying the cold gas mass in these filaments across ionised\, molecular\, and atomic phases\, we estimate the energy required for feedback to lift this material. We relate star formation in the disk to the energy associated with feedback. Our results can directly inform sub-grid physics for galaxy evolution simulations and serve as a benchmark for large surveys of single-phase wind measurements. They also emphasise the critical role of multi-wavelength approaches in the upcoming SKA era.vent here … \n\n\nMS Teams\n\n\nkensington\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/barbara-mazzilli-ciraulos-colloquium/
LOCATION:26 Dick Perry Ave\, Kensington WA 6151\, 26 Dick Perry Avenue\, Kensington\, Washington\, 6151
CATEGORIES:Colloquia
ORGANIZER;CN="Nikhel Gupta":MAILTO:nikhel.gupta@csiro.au
END:VEVENT
END:VCALENDAR