. Tabella L1 (in EURO ) . (vedi Tabella in Lire ) . STIPENDI TABELLARI . (in lire per 12 mensilitЮ) . Fascia stipendiale . dal 1.7.00 . I . II . III . da 0 a 4 . 32.034,27 . 23.239,01 . 16.863,35 . da 5 a 8 . 36.493,88 . 26.485,46 . 19.167,78 . da 9 a 12 . 41.118,75 . 29.783,55 . 21.516,11 . da 13 a 16 . 45.713,15 . 33.069,77 . 23.839,13 . da 17 a 22 . 52.207,08 . 37.644,54 . 27.145,49 . da 23 a 30 . 58.533,68 . 42.215,19 . 30.398,65 . da 31 in poi . 66.733,98 . 48.062,00 . 34.562,33 .
. Space Telescope Science Institute . help@stsci.edu . Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Appendix A: ImagingReference Material > Camera 1, Filter F145M . Camera 1, Filter F145M . Notes: . H 2 O band. Central wavelength: 1.4546 ? m . Mean wavelength: 1.4558 ? m . Peak wavelength: 1.5100 ? m . Wavelength range: 1.35?1.55 ? m . FWHM: 0.1963 ? m . Maximum throughput: 18.233% . Central pixel fraction: 0.057 . Figure A.9: NIC1, F145M Throughput .
Supernova 2009ip in NGC 7259 . This page is devoted to information on Supernova 2009ip in NGC 7259 . ... In July 2012, CRTS noticed that this object had started to brighten again. ... Then in September of 2012 it got brigher again. ... Cornell University The Unprecedented Third Outburst of SN 2009ip: A Luminous Blue Variable Becomes a Supernova . ... UIS Henry Barber Research Observatory 2009ip page . ... 2009/08/26.11 . ... Joseph Brimacombe . ... Stan Howerton . ... Stan Howerton Light curve . ...
Supernova 2004dt in NGC 799 . This page is devoted to information on Supernova 2004dt in NGC 799 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. ... 2004/08/11.480 . ... Light curves and Spectra: . CSP optical light curve . SNWeb Measurements and light curve . VSNET Light curve (requires JAVA). ...
Известные данные о распределении спутниковых орбит и кольцевых структур в системах больших планет (и планет, астероидно-кометных тел в Солнечной системе) позволили выявить иерархическую поясную структуру расположения орбит компаньонов. Как и планеты Солнечной системы спутники больших планет (и их кольцевые структуры) объединяются в группы (обозначим их (r, A, B, C, D, E)). ... Разницы больших полуосей для соседних компаньонов одной группы являются одинаковыми. ...
Computer Ephemeris for 2015 from DE200/LE200. Reduction quantities ( dynamical time scale). tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Jan 1 -0.5007 -8.096 9.541 -3.415 20.491 7 -53 21 2 -0.4979 -8.013 9.568 -3.742 20.422 7 -37 52 3 -0.4952 -7.920 9.582 -4.067 20 tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Feb 1 -0.4158 -6.115 9.174 -12.598 15.600 8 43 72 2 -0.4131 -6.041 9.138 -12.843 15.356 8 65 55 3 -0.4103 -5.978 9.092 -13.084 15 ...
STRUCTURE AND CYCLIC VARIATIONS OF OPEN MAGNETIC FIELDS IN THE SUN V. N. OBRIDKO and B. D. SHELTING IZMIRAN, 142092, Troitsk, Moscow Region, Russia (Received 28 October 1997; accepted 2 March 1999) Abstract. The structure and variations of open field regions (OFRs) are analyzed against the solar cycle for the time interval of 1970 1996. ... This supports the concept of a single complex `large-scale magnetic field active region coronal hole'. ... Butterfly' diagram of the open field. ...