Search

13 Mar 2012: Photon easy to detect and measure! [GeV]Tγp. 200 300 400 500 600 700. ... n=4.0 0.6 - 1.0!•MPL = 1029 200 - 100 GeV! 3/12/12 Astroparticle 23.

10 Feb 2012: He took with him an overview of what VST data for 200 band-merged ATLAS fields currently yields.

5 Oct 2012: γ Tri 70 777.638.8 21.200.40 756.438.8 40 10.240.04100 718.835.5 10.290.20 708.535.5 40 11.630.04160

23 Oct 2012: 2006) and the effective. temperature of the large rubble, 200 K, they placed the dust populations at 5.8 0.6 (1) AU. ... fine dust” are much better at radiating heat and needs only to reach a color temperature of 200.

19 Jun 2012: Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed 18 June 2012 (MN LATEX style file v2.2). Debris from terrestrial planet formation: the Moon-forming collision. Alan P. Jackson1? and Mark C. Wyatt1?1Institute of Astronomy, University of Cambridge,

7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars.

12 Jan 2012: 57,PA = 3171 , ρ = 1.200.014”). ... An object in such an orbit would havea period of at least 200 years, so could not have been detectednear the star in 2005 and be outside the NIRC2 field of

9 Oct 2012: Coplanar Circumbinary Debris Disks 11. 0 50 100 150 200 250 300Semi-major axis (AU).

29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.

1 Aug 2012: The mass of fine dust is 4 1019–2 1020 kg, equivalentto a 150–200 km radius asteroid. ... a very large particle dust population (a > 100 μm), radiatingas blackbodies at 200 K.