Search

19 Apr 2006: Dominik,5 and H. J. Walker6. Received 2004 September 17; accepted 2004 December 20; published 2005 January 10. ... The total dust flux within a diameter circle is′1 37.0mJy at 850mm and mJy at 450mm, in good2.5 250 20.

27 Jun 2006: The resulting distance moduli are: dmag = [18.2, 20.9, 16.8] In principle, from the CMD matching, you can't really shift the ridgeline by more than 0.05 mag

19 Apr 2006: The diameter of theP.A. = 1757 5 107major axis of the emission at 10.8 mm is 20.2, which corre-sponds to 215 AU. ... At 18.2 mm the maximum extent of theemission is 20.0 (198 AU), which is about 90% the size ofthe 10 mm emission.

17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

19 Apr 2006: wing along lines through the star. The nine evenly spaced contour levels are at the 10, 20,. ... We ignore results for the regionwithin 20 AU of the star because of the contribution of the silicate feature and uncertaintiesin the PSF.

26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

19 Apr 2006: Received 2002 April 17; accepted 2002 September 20. ABSTRACT. New submillimeter images of the cold dust emission around the nearby main-sequence star Fomalhaut arepresented. ... mJy beam1). Integrated Fluxb. (mJy). 450. 7.1, 12.3 119 20 7.4, 16.2 124 20

8 Mar 2006: 4400. 22.1. 2.6. V. 5500. 21.3. 3.5. R. 6000. 20.4. 3.9. ... 3000. 22.0. 21.2. 20.0. 19.5. 100. Galactic Plane Magellanic Clouds. 1500.

19 Apr 2006: Combining this with the beam size, the effectiveresolution is 20 arcsec or 70 au. ... Figure 1. 850-µm image of τ Ceti, smoothed to 20-arcsec resolution.

15 Apr 2006: 0.10. V. 5500. 21.3. 21.4. 9.6. 3.5. 0.15. R. 6000. 20.4. ... In some the star–formation at this level may have begun at z10-20.

2 Nov 2006: The above plots are all in the WFCAM instrumental system and the 5-sigma limiting magnitudes for stellar objects in this data in this system are approximately Y = 20.9, J = ... 20.6, H = 19.8, K = 19.1 ,all in a Vega system.

17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in yamounting to 0.05 pixel (20 mas) over the observed magnitude range.

26 May 2006: m. 20.3. s. 48 31' 40" and has a 2MASS J magnitude of 8.79. ... The individual frames are 20 second exposures taken in Z. About 20 seconds elapse from the end of 01867 and the start of 01868.

19 Apr 2006: Consideration of the collisional lifetime of different sizedbodies in the disk showed that what we are seeing is just the bottom half of the cascade(7 µ m dust to 20 ... C., and Taidakova, T. A., Astrophys. J., 537, L147–L151. (2000).20. Macintosh, B.

19 Apr 2006: 0. 20. 40. Ecl. ipti. c L. atit. ude. 70 80 90 100 110Ecliptic Longitude Relative to Sun. ... 40. -20. 0. 20. 40. 70 80 90 100 110Ecliptic Longitude Relative to Sun.

16 Nov 2006: predominantly Mg-rich olivines (80%) and crystalline pyroxenes (20%) (Figure 3). Unlike our. ... Dark blues - crystalline olivines, forsterite and fayalite, in order of 20 µm amplitude.

19 Apr 2006: areconsistent with a ring of radius 150 20 AU seen at 45 25 inclination. ... would migrate from 150to 0 AU (where it would evaporate) on timescales of 20 Myr(Burns et al.

19 Apr 2006: and Spangler et al. (2000) are also included here – ISO observed 70per cent of the single A stars but only 20 per cent of single G starswithin 25 pc. ... If the r 3 line in Fig. 2 is extrapolatedfrom 20 to 25 pc, the detections should increase to 20

14 Dec 2006: 2004).These two stars are 10–20 Myr old (see Favata et al. ... 1 AU) while (sub)mm surveys probe cold dust (20 K)distant from the star (100’s AU).

6 Jun 2006: The proposed VHS survey will have a 10σ limit in Y of 20.4[Vega]; see Table 1. ... UKIDSS LAS uses SDSS z’ with a median 5σ limit(Vega) of 20.3.