Web services based workflows to deal with 3D data
VO web-services-based astronomy workflows
Formation of Massive Stars With great advances achieved in our understanding of low mass star formation, it is tempting to think of high mass star formation.
Taurus: Then and Now Susan Terebey CSULA Dept of Physics & Asronomy Dense Cores in Dark Clouds LXV for Phil Myers 21 October 2009.
Ammonia and CCS as diagnostic tools of low-mass protostars
Astrometry from VERA to SKA
Super Massive Black Holes Outstanding synergy with Fermi -ray telescope…same particles produce -rays also radio photons. While -rays may dominate.
Allen et al. (2005)
AGNs with the VLTI. Cygnus A:I What’s an AGN What’s an AGN? (L = 10^46 erg/s) Radio Jet (sometimes) @ 300 kpc Narrow Line Region @ 1 kpc [dusty torus/disk@1pc]
The Galactic Australia SKA Pathfinder Spectral Line Survey (GASKAP) Hiroshi Imai Graduate School of Science and Engineering, Kagoshima University International.
EVLA Status --
Super Massive Black Holes
![AGNs with the VLTI. Cygnus A:I What’s an AGN What’s an AGN? (L = 10^46 erg/s) Radio Jet (sometimes) @ 300 kpc Narrow Line Region @ 1 kpc [dusty torus/disk@1pc]](https://static.fdocuments.us/doc/330x215/56649c6a5503460f94918647/agns-with-the-vlti-cygnus-ai-whats-an-agn-whats-an-agn-l-1046.jpg)
