... This paper describes a James Clerk Maxwell Telescope (JCMT) legacy sur vey that has been awarded roughly 500 hr of obser ving time to be carried out from 2007 to 2009. In this sur vey, we will map with SCUBA2 (Submillimetre Common-User Bolometer Array 2) almost all of the well-known low-mass and intermediate-mass star-forming regions within 0.5 kpc that are accessible from the JCMT. ... 2007). ... To test the predictions of low-mass star formation theories (core, outflow, field geometr y). ...

Еще в разделе: (Показать все результаты (>5) - www.mrao.cam.ac.uk/ )

• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf
• http://www.mrao.cam.ac.uk/~eic22/Papers/curtisricher_scuba.pdf
• http://www.mrao.cam.ac.uk/~eic22/Papers/curtisricher2010b.pdf

ATNF ATUC MEMORANDUM To: ATUC From: Michael Burton Date: 2 June 2004 Subject Draft of a major project for Mopra To assist in the discussion of possible key projects that Mopra could be used for, attached is a draft of a proposal to perform a large multi-line survey to help constrain star formation models. The (-Quadrant Survey Turbulence-regulated Star Formation? ... The necessary molecular can be obtained using the Mopra Telescope through the (-Quadrant Survey. ...

Еще в разделе: (Показать все результаты (>6) - www.atnf.csiro.au/ )

• http://www.atnf.csiro.au/management/atuc/2006jun/docs/8_mmwhitepaper.pdf
• Sims Workshop Abstracts

How Dry is the Brown Dwarf Desert?: Quantifying the Relative Number of Planets, Brown Dwarfs and Stellar Companions around Nearby Sun-like Stars Daniel Grether1 Charles H. Lineweaver 1 1,2 arXiv:astro-ph/0412356 v1 15 Dec 2004 Department of Astrophysics, School of Physics, University of New South Wales, Sydney, NSW 2052, Australia Planetary Science Institute, Research School of Astronomy and Astrophysics Research School of Earth Sciences, Australian National University ... 4ґ Fig. ...

Еще в разделе: (Показать все результаты (>2) - www.mso.anu.edu.au/ )

• http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver06.pdf

Rep ort by the ESA-ESO Working Group on Galactic p opulations, chemistry and dynamics Abstract Between the early 40s, when Baade showed the first evidence for the existence of two distinct stellar populations, and today, with our Galaxy surprising us with new substructures discovered almost on a monthly basis, it is clear that a remarkable progress has been achieved in our understanding of the Galaxy, of its structure and stellar populations, and of its chemical and dynamical signatures. Yet, some questions

Еще в разделе: (Показать все результаты (>2) - www.stecf.org/ )

• http://www.stecf.org/coordination/esa_eso/extrasolar/report.pdf