Search

Search Funnelback University

Search powered by Funnelback
10 results 20 results 50 results
Relevance Date (Newest first) Date (Oldest first) Title (A-Z) Title (Z-A) Distance URL (A-Z) URL (Z-A) Shuffle
1 - 10 of 10 search results for KaKaoTalk:po03 op |u:people.ast.cam.ac.uk where 0 match all words and 10 match some words.

  1. Results that match 1 of 2 words

  2. ��������� ��� �������� �� ������������� ��� "!# $�&% '�…

    https://people.ast.cam.ac.uk/~wyatt/wyat03a.pdf
    19 Apr 2006: "!# $&% ' )(# -,/.0-%12 &!$3542,67,98/:<;=?> @A>BDCFEGIHJ8K>L>MONPEQRCFSUTV8WX>YZ>L[GIEE]E[_7=?>Ya>bCFcXdGIHe_UNPEgfMhC[cA:QUeiPGkjEmlPG#QU_UmSn;opQqGI_U_#8rMhC[cX:Qq]iPG$st8vuFwPwPx>yopzV>|{-}8vuP{}Ic>yopQU]#GpPwgfT2C[Qqi:NPdEiV9bKhw{Pu&}&}P<As>.

  3. arX iv:a stro -ph/ 0603 608 v2 1 Se ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/dye.pdf
    28 Sep 2006: arX. iv:a. stro. -ph/. 0603. 608. v2. 1 Se. p 20. 06. Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 4 September 2006 (MN LATEX style file v2.2). The UKIRT Infrared Deep Sky Survey Early Data Release. S. Dye1, S. J. Warren2, N. C. Hambly3, N.

  4. ��������� �� ��������������������� �������� ����������� "!…

    https://people.ast.cam.ac.uk/~wyatt/wdt00.pdf
    19 Apr 2006: "! $#&%(')! ,.-/%103246587797: 0<;=>&?%/3#60A@ B4%)CD0CEGFHI6KJ&0ML80ONPRQ8%S 4T0. UWVYXOZ [MV6]AXV_ba c&dfehgjiZ k.l<]m.XOV$c=nPo$Zpp.V6qUhal VC]rsZ qoftuvxw=y"z. {}|x|C) 9(A6Wf69O6AR.E&RAAA9E9 //.¡¢E£¤E(¥ª«¢¥ª<E4OP/GK=. |Y|&µEºA)»|&{f|

  5. arX iv:a stro -ph/ 0601 592 v1 26 J ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf
    28 Sep 2006: The low sensitivityof most optical CCD detectors at 1 µm, coupled with therelatively bright sky-background curtailed interest from op-tical astronomers.

  6. ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf
    19 Apr 2006: ApJ accepted, 7 November 2005Preprint typeset using LATEX style emulateapj v. 04/21/05. DUST IN RESONANT EXTRASOLAR KUIPER BELTS — GRAIN SIZE AND WAVELENGTH DEPENDENCEOF DISK STRUCTURE. M. C. Wyatt1. UK Astronomy Technology Centre, Royal

  7. SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...

    https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf
    19 Apr 2006: 4.2. Modelingg the SED. The spectral energy distribution (SED) of Corvi from op-tical to submillimeter wavelengths is plotted in Figure 4.

  8. ��������� �� ���������������������������������!…

    https://people.ast.cam.ac.uk/~wfcam/ukreview/wfcam_instrument.pdf
    28 Sep 2006: tuwv »¿ x v , v &,-3'T$É!' v $%3& v x2#AÎG&ÖP-!1Y, uwv x v |, v &,-3'i3&(,) yGv 3' v )s%.;.

  9. ����������� ��� ������������ ������� �!�"���…

    https://people.ast.cam.ac.uk/~wyatt/wyat05a.pdf
    19 Apr 2006: " $#%&%&' ()" #$%%'-,.0/(12&34657798:";" =<>? @$$A$>;"? BC? ";D= ;" EF46 "9/ GHJI"K"KMLBNPOQ R9SOETUQ VFW"OXTMY!Z[QS W"OXW"]BV. GTMY_OXVFW"O. (a Nb?K"K&c K"K"K"KdUe(K"K"K"K"K"K"K"K"K"K"K"K"K"K"KMe. fhgji kmlon_pqnsr turwv xzy|{|}ns{|r {|wi}_. 6sJ

  10. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: To probe the nature of the Vega disk further, wehave fitted it with models including realistic grain op-tical properties.

  11. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: 10 µm) to spiral inwards toward the star.Which of these two effects is dominant depends on the op-tical depth of the dust disk, but for all but the most

Refine your results

clear all

Date

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.