... The 7227 candidate list contains 31M-dwarf stars which are (a) nearby (d 6 pc) with spectral types later than M3.5, (b) young (age 100 Myr) with (d 25 pc), and (c) spectrally the latest known (i.e.,``ultra-cool" stars later than M8.5), with some overlaps ...
... Final programme . TUESDAY 29 May . WEDNESDAY 30 May . THURSDAY 31 May . FRIDAY 1 June . POSTERS All Sessions. ... Roeland v/d Marel . M/L Evolution and Formation Redshift of Elliptical Galaxies . 15.00 15.20 . Jesus Falcon Barroso . ...
... Fig. 2 shows the images of HD 97300 obtained in the four CAM narrow-band filters centered at 6.0 m (lw4), 6.8 m (lw5), 11.3 m (lw8) and 14.9 m (lw9). ...
... REFER E NC ES Almaini O., Boyle B. J., Griffiths R. E., Shanks T., Stewart G. C., Georgantopoulos I., 1995, MNRAS, 277, L31 Antonucci R., 1993, ARA&A, 31, 473 Bertin E., Arnouts S., 1996, A&AS, 117, 393 Binney J., Merrifield M., 1998, Galactic Astronomy. ...
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Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/croom01.pdf -- 588.2 Кб -- 16.09.2004 Похожие документы
... U. Becciani, V. Antonuccio-Delogu, M. Gambera and A. Pagliaro . ... The most popular algorithms are generally based on grid methods like the P 3 M . ... 1Mun_tf_bc . 128 . 4875 . 186.31 . 205.32 . 4.14 . 1Mcl_tf_bc . ...
... 2 ST-ECF Instrument Science Report ACS 2001-004 WFC grism stamp image is shown in Figure 1; it includes both the 1st and 2 tra of CJFN #1, #31 and JC #57. nd order spec- JC #57 CJFN #31 CJFN #1 Figure 1: The 1st and 2 nd order grism simulated WFC spectra ...
... U. Becciani, V. Antonuccio-Delogu, M. Gambera and A. Pagliaro Osservatorio ... The most popular algorithms are generally based on grid methods like the P 3 M . ... FC phase 230.05 250.32 270.51 291.63 186.31 203.37 1051.93 1173.24 T-step 249.5 268 ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/beccianiu.pdf -- 134.4 Кб -- 12.06.2006 Похожие документы