How Do Stars Form?
general audience · 27 stops
The Ginsburg group’s research told as a story, from the Galactic Center to individual protostars, with the students behind each result.
Guided tours through the Ginsburg group’s data at the University of Florida: ALMA, JWST, VLA, and single-dish views of star formation in the Galactic Center and the disk. Each tour flies between positions in Aladin Lite, fading between image layers as it goes.
Press Open to step through a tour yourself, or Full screen
for a kiosk view that plays on its own — useful on a display in the hallway.
Add ?random=true to start at a random stop.
general audience · 27 stops
The Ginsburg group’s research told as a story, from the Galactic Center to individual protostars, with the students behind each result.
colloquium · 35 stops
The technical version: ACES, JWST, and VLA/ALMA results on the CMZ, Sgr B2, W51, and the young massive clusters.
talk / interactive · 8 stops
JWST and ALMA on the same three fields, from Nazar Budaiev’s CARTA figure. Click a white box to zoom into it, or let it play through.
talk · 7 stops
Spitzer to ACES to JWST: the Central Molecular Zone, the ACES footprint, then a zoom into one dust-ridge cloud.
talk / general audience · 16 stops
Four unexplained things in the Galactic Center: the MUBLO, the “fluff” in Sgr B2, the “smudge” in Cloud C, and the ionized streaks.
survey · 28 stops
The ALMA CMZ Exploration Survey across the Galactic Center, molecule by molecule.
survey · 24 stops
Early ACES science: the line mosaics and what each tracer picks out.
survey · 13 stops
JWST NIRCam and MIRI coverage of the Galactic Center clouds.
region · 10 stops
The most active star-forming cloud in the Galaxy at infrared and millimeter wavelengths.
region · 63 stops
A massive protocluster in the disk: JWST colors over VLA and ALMA continuum.
region · 8 stops
A young massive cluster, JWST NIRCam and MIRI compared with HST.
general audience
A wide sweep of JWST star-formation images, from Orion outward.
general audience
Protostellar jets and the shocks they drive into their parent clouds.
survey
Single-dish submillimeter coverage of the CMZ handing off to the ALMA mosaic.
slider · 1 stops
Slide through JWST filters on G0.253+0.016, linear stretch.
slider · 1 stops
The same filter set with logarithmic and alternative scalings.
slider · 1 stops
JWST filters across Sgr B2, linear stretch.
slider · 1 stops
Sgr B2 with logarithmic and alternative scalings.
slider · 1 stops
The Sickle near the Quintuplet cluster, linear and logarithmic.
slider · 1 stops
JWST filters across W51, linear stretch.
slider · 1 stops
W51 with logarithmic and alternative scalings.
slider · 1 stops
W51 filter triplets from the pipeline residual mosaics, fitted stars removed.
slider · 1 stops
Every adjacent JWST filter triplet across Westerlund 2, F115W to F1130W.
slider · 1 stops
Adjacent JWST filter triplets across the Sickle, F187N to F1500W, linear stretch.
slider · 1 stops
Adjacent filter triplets across the Arches cluster, F212N to F770W.
slider · 1 stops
Adjacent JWST filter triplets around Sgr A*, F115W to F1500W.
slider · 1 stops
Adjacent NIRCam filter triplets across Sgr C, F115W to F480M.
slider · 1 stops
Adjacent JWST filter triplets across Clouds E and F, F162M to F2100W.