Search
Search Funnelback University
31 -
40 of
350
search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk
where 0
match all words and 350
match some words.
Results that match 1 of 2 words
-
arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest -
Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …
https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf18 Apr 2022: 11 174718. 11910 123109310. 638406 245. Number of detectable planets. 0 200 400. ... Sub-Neptunes Sub-Jovians0. 50. 100. 150. 200. 250. 300. 350. Det. ecta. -
Chapter 2 - Operating the software
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically. -
MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf13 Jul 2016: 0 100 200 300 400 500. UV Distance [kλ]. 100. 0. ... 100. 200. 300. Re(v. ) [m. Jy]. 0 100 200 300 400. -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU). -
Debris discs around nearby solar analogues
https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf8 Jul 2009: e. upto approximately 200 au radius for stars at 12–15 pc distance. ... For five precise (G2 V) solar analogues,the fitted disc radii are 100–200 au (Krivov et al. -
MGB thesis Chapter 3
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design, -
L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...
https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 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.
Refine your results
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
- `Jim Watson` |u:www2.mrc-lmb.cam.ac.uk (0) · moments ago
Recent searches
Your search history is empty.