... The alloy with x = 0.171 is found to deviate from the linear Curie point dependence on pressure. The interrelation between the magnetic T-C diagram peculiarities and the anomalies of the thermal expansion coefficient and the isotherm of the magnetic susceptibility in the paramagnetic range is investigated. ... 5, Tc and T, decrease linearly with increasing pressure. ... It is seen in Fig. 2 that the P(Tc)dependence for the alloy KO. is nearly 5 parabolic in the investigated temperature range. ...

Supernova 1999em in NGC 1637 . This page is devoted to information on Supernova 1999em in NGC 1637 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main main page . Information on the original web pages for many of these images can be found on the Supernova links web page. ... LOSS image . ... vsnet-alert 3639 ] SN 1999em in NGC 1637 . vsnet-alert 3640 ] SN 1999em in NGC 1637 . ... vsnet-recent 39999 ] SN1999em recent (cont'd) . ...

... mag . ... 127 points . ... mag(J4)-mag(J2) . ... 1012 points . ... mag(J2+J3)-(mag(J1)+(mag(J4))/2 . ... 79 points . 084 Pulkovo . ... 536 points . ... mag(J3+J4) without reference object, quadratic trend is deleted . ... 475 points . ... 26-inch refractor . ... 1124 points . ... 1272 points . ... 395 points . ... 628 points . ... 391 points . ... 777 points . ... 458 points . ... mag(J1+J3)-mag(J2), united with 3E1 . ... mag(j1+j3)-mag(star) . ... 4.6 . ... mag(J1)-(mag(J2)+mag(J3)+mag(J4))/3 . ...

... Grechnev,б V.б V.; Kiselev,б V.б I.; Meshalkina,б N.б S.; Chertok,б I.б M. Relations Between Microwave Bursts and Near-Earth High-Energy Proton Enhancements and Their Origin . ... Chertok,б I.б M.; Belov,б A.б V.; Grechnev,б V.б V. A Simple Way to Estimate the Soft X-ray Class of Far-Side Solar Flares Observed with STEREO/EUVI . ... Fomichev,б V.б V.; Chertok,б I.б M. Comparison of data on proton fluxes at the earth with results on the diagnostics of solar proton flares according to radio bursts . ...

... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...

Astronotes Armagh Planetarium's Stellar Blog! ... By admin September 26, 2011 Posted in: Cosmology . ... Neutrinos emitted by this explosion did not travel faster than light. ... Albert Einstein (1879-1955) came up with the theory of relativity that established the speed of light as the cosmic speed limit. ... If you divide the distance between those two points by the time it takes for the neutrinos to travel, you get their speed. ... Reply . ... Posted September 26, 2011 at 3:41 PM . ... Astronotes . ...

CHAPTER 12: Lead Center Space Center personnel began work on the Space Shuttle under the cloud of reductions in force, tightening budgets, growing public apathy or outright criticism, and unclear and changing program directives. ... Budgetary constraints contributed to the decision to establish a lead center management approach for the Shuttle and affected program development. ... Now, as Shuttle Program Manager, Thompson had overall responsibility for the development of the Shuttle. ...