Jessica R. Lu Institute for Astronomy University of Hawaii

More documents

Recommendations

Info

Current AO systems have too small FOV. Gemini MCAO - ideal system for clusters at 3 - 10 kpc JWST - ideal for characterizing unresolved clusters in other galaxies need bigger FOV for nearby massive clusters (especially lower metallicity outer Galaxy clusters) still need good resolution for precise astrometry moderate resolution spectroscopy for many objects
Stars in formation in motion
Page 1 and 2: Stars in formation in motion Jessic
Page 3 and 4: 10 5 M sun 10 4 M sun 10 3 M sun
Page 5 and 6: Massive young clusters are difficul
Page 7: Current AO systems have too small F
Page 11 and 12: Successful pilot project for W51. D
Page 13 and 14: Currently, relative astrometry is p
Page 15 and 16: Slides Internal Save As: dynamics j
Page 17 and 18: Masses of stars, brown dwarfs, and
Page 19 and 20: Astrometric microlensing can probe
Page 21 and 22: Astrometric microlensing can probe
Page 23 and 24: Astrometry is relevant to many addi

Jessica R. Lu Institute for Astronomy University of Hawaii

Create successful ePaper yourself

Delete template?

Save as template?