By Jose Afonso, Nuno Santos, Andre Moitinho, Rui Agostinho
Read or Download 2005: Past Meets Present in Astronomy And Astrophysics: Proceedings of the 15th Portuguese National Meeting PDF
Best mathematicsematical physics books
This booklet, "Project Physics source Book", by means of F. James Rutherford, Gerald Holton, and Fletcher G. Watson, is a replication of a ebook initially released prior to 1981. it's been restored by way of humans, web page through web page, so you could take pleasure in it in a sort as with regards to the unique as attainable. This ebook was once created utilizing print-on-demand know-how.
In March 2001, the nationwide Institutes of health and wellbeing issued the subsequent caution: "The variety of websites providing health-related assets grows on a daily basis. Many websites offer helpful info, whereas others could have info that's unreliable or deceptive. " additionally, a result of quick elevate in Internet-based details, many hours might be wasted looking, making a choice on, and printing.
- The Harvest of a Century: Discoveries in Modern Physics in 100 Episodes
- Scientific Detectors for Astronomy 2005 : Explorers of the Photon Odyssey (Astrophysics and Space Science Library)
- Neutrino Geophysics: Proceedings of Neutrino Sciences 2005
- Physical Theory and its Interpretation: Essays in Honor of Jeffrey Bub (The Western Ontario Series in Philosophy of Science)
- Growth, Physical and Motor Development in Prepubertal Children (Exercise Physiology)
Extra info for 2005: Past Meets Present in Astronomy And Astrophysics: Proceedings of the 15th Portuguese National Meeting
Astron. 52, 115 (2002) PROBING THE STRUCTURE A N D ATMOSPHERES OF EXTRA-SOLAR PLANETS N. C. pt In this paper we review the recent results concerning the detection of extra-solar planets, with particular emphasis on the cases where a transit event is measured. 1. I n t r o d u c t i o n From 1995 to the present, following the discovery of the first extra-solar planet orbiting a solar type star 1 6 , about 160 giant planets have been announced, showing t h a t these are common around stars in the solar neighborhood 3 '.
In this section we report the results of DAOSPEC in a big sample composed of 62 stars. 000, s/n ~ 200 - 400), on October 2004. The lines used to do this test are standard Fe I and Fe II lines used to determine stellar parameters. A list of this lines can be found in Santos et al. (2004). One of the parameters of DAOSPEC is the wavelength interval for the calculation. Using the full individual spectrum interval yielded a large dispersion of the measurements. This comes from the fitting of the continuum level and, therefore, we considered small intervals, 500A wide, instead.
A&A 417, 353 (2004) 10. Gaudi, B. , ApJ 623, 472 (2005) 11. , Annual Review of Earth and Planetary Sciences 33, 493 (2005) 12. , A&A 431, 1129 (2005) 13. Henry, G. , Marcy, G. , Butler, R. , and Vogt, S. , ApJ 529, L41 (2000) 14. , Nature, 421, 507 (2003) 15. , Sasselov, D. , ApJ, 624, 372 (2005) 16. Mayor, M. , Nature 378, 355 (1995) 17. , MNRAS 356, 955 (2004) 18. , ApJ 614, L81 (2004) 19. , A&A 426, L15 (2004) 20. , A&A 433, L21 (2005) 21. , A&A 438, 1123 (2005) 22. Santos, N. , A&A 373, 1019 (2001) 23.
2005: Past Meets Present in Astronomy And Astrophysics: Proceedings of the 15th Portuguese National Meeting by Jose Afonso, Nuno Santos, Andre Moitinho, Rui Agostinho