Resolving such imbalances requires either a manifestly artificial ' world ', or metagame constructs such as hit points, level adjustments, etc.

Resolving to seek no knowledge other than that of which could be found in myself or else in the great book of the world, I spent the rest of my youth traveling, visiting courts and armies, mixing with people of diverse temperaments and ranks, gathering various experiences, testing myself in the situations which fortune offered me, and at all times reflecting upon whatever came my way so as to derive some profit from it.

Resolving contradictions, perceived or actual, between different statements in the Mishnah, or between the Mishnah and other traditions ; e. g., by stating that: two conflicting sources are dealing with differing circumstances ; or that they represent the views of different Rabbis.

The second book, Crucial Confrontations: Tools for Resolving Broken Promises, Violated Expectations, and Bad Behavior, McGraw-Hill, 2005, teaches important skills for dealing with accountability issues.

Resolving to devote himself and his means wholly to the advancement of Christianity, his first proposal for that end, made in 1796, was to organize a vast mission to Bengal, of which he was to provide the entire expense ; with this view the greater part of his estate was sold, but the British East India Company refused to sanction the scheme, which therefore had to be abandoned.

* Healing the Planet: Strategies for Resolving the Environmental Crisis ( 1991, co-authored with Anne Ehrlich )

* 2000-04: WALID Inc. ( with IDNA patent pending application 6182148 ) started Registration & Resolving Multilingual Domain Names.

In January 2011 he launched a consultation: ' Resolving Workplace Disputes ', jointly with Ed Davey MP ( who at the time was a Business Minister ).

Resolving the 16 double points of the quotient of a ( possibly nonalgebraic ) torus by the Kummer involution gives a K3 surface with 16 disjoint rational curves ; these K3 surfaces are also sometimes called Kummer surfaces.

* with John Gerhart, The Plausibility of Life: Resolving Darwin's Dilemma ( Yale University Press 2005 ) ISBN 0-300-10865-6

Resolving to get something done, I started in on the dishes.

Resolving usually entails iterating through several name servers to find the needed information.

* Extraterrestrial Intelligence in the Solar System: Resolving the Fermi Paradox by Robert A. Freitas Jr.

Resolving a flame war can be difficult, as it is often hard to determine who is really responsible for the degradation of a reasonable discussion into flame war.

Resolving to release his mother from this state of bondage, Garuda approached the serpents and asked them what it would take to purchase her freedom.

* A. Chorti and M. Brookes ( 2007 ), " Resolving near-carrier spectral infinities due to 1 / ƒ phase noise in oscillators ", ICASSP 2007, Vol.

Resolving these issues delayed the first night until 3 March 1875 on which morning, by chance, Bizet's appointment as a Chevalier of the Legion of Honour was announced.

Resolving these two states in a believable way can be quite complex.

* Resolving Sexual Abuse: Solution-Focused Therapy and Ericksonian Hypnosis for Adult Survivors by Yvonne M. Dolan ( WW Norton & Company: New York, 1991 ).

Resolving this discrepancy is one of the foremost problems in astronomy since the cosmological parameters of the Universe may be constrained by supplying a precise value of the Hubble constant.

Resolving a Historical Confusion in Population Analysis.

Resolving the accounts is a matter tied to the synoptic problem.

Resolving social conflicts.

Resolving power is the ability of an imaging device to separate ( i. e., to see as distinct ) points of an object that are located at a small angular distance.

* One State, Two States: Resolving the Israel / Palestine Conflict, Yale University Press, 2009.

If components in binary star systems are close enough they can gravitationally distort their mutual outer stellar atmospheres.

If a star grows outside of its Roche lobe too fast for all abundant matter to be transferred to the other component, it is also possible that matter will leave the system through other Lagrange points or as stellar wind, thus being effectively lost to both components.

Studies of the eclipsing ternary Algol led to the Algol paradox in the theory of stellar evolution: although components of a binary star form at the same time, and massive stars evolve much faster than the less massive ones, it was observed that the more massive component Algol A is still in the main sequence, while the less massive Algol B is a subgiant star at a later evolutionary stage.

Their measurement of γ Virginis in 1718 was the first made of the components of a double star and was directed towards the determination of stellar parallax.

These are thought to form in stellar nurseries, and quickly fragment into stable multiple stars, which in the process may eject components as galactic high velocity stars.

After duty supplying optical components to the military in World War II, the emphasis on astronomical research changed in the late 1940s from solar to stellar research.

The two brightest components are metallic-lined subgiant stars belonging to the A-type stellar classification ; they have roughly the same mass and radius.

Thus, observations of binary stars where the two components are at such different stages of stellar evolution can be used to determine the relationship between the mass of stars and how they evolve.

To explain stellar aberration in the context of an aether-based theory of light was regarded as more problematic, because it requires that the aether be stationary even as the Earth moves through it — precisely the problem that led Newton to reject a wave model in the first place.

( The latter criterion requires some knowledge of the relevant pressures in the stellar atmospheres, and Saha following the generally accepted view at the time assumed a value of the order of 1 to 0. 1 atmosphere.

The stellar movement proved too insignificant for his telescope, but he instead discovered the aberration of light and the nutation of the Earth ’ s axis.

When James Bradley and Samuel Molyneux entered this sphere of astronomical research in 1725, there consequently prevailed much uncertainty whether stellar parallaxes had been observed or not ; and it was with the intention of definitely answering this question that these astronomers erected a large telescope at the house of the latter at Kew.

In 1921 Albert A. Michelson made the first measurements of a stellar diameter using an interferometer on the Hooker telescope.

The stellar disks he observed were spurious ( likely the Airy disk caused by diffraction, as stars are too distant for their physical disks to be detected telescopically ), but Marius interpreted them to be physical disks, like the planetary disks visible through a telescope.

He concluded that since he could see stellar disks, the stars could not be as distant as was required in the Copernican world system, and he said that the appearance of the stars as seen through a telescope actually argued against Copernicus.

The stellar movement proved too insignificant for his telescope, but he instead discovered the aberration of light, the nutation of the Earth ’ s axis, and did a cataloging of 3222 stars.

By means of a water-filled telescope, Airy in 1871 looked for a change in stellar aberration through the refracting water due to an ether drag.

" However, after the advent of the telescope showed problems with some geocentric models ( by demonstrating that Venus circles the sun, for example ), the Tychonic system and variations on that system became very popular among geocentrists, and the Jesuit astronomer Giovanni Battista Riccioli would continue Tycho's use of physics, stellar astronomy ( now with a telescope ), and religion to argue against heliocentrism and for Tycho's system well into the seventeenth century ( see Riccioli ).

A transmission grism is a useful component in an astronomical telescope, allowing observation of stellar spectra.

* December 13-The red giant star Betelgeuse is the first to have its diameter determined by an optical astronomical interferometer, the Michelson stellar interferometer on Mount Wilson Observatory's reflector telescope.

Other objects can be observed using CCD cameras or photoelectric photometers connected to a telescope, and the flux, or amount of light received, can be compared to a photometric-standard star to determine the exact brightness, or stellar magnitude, of the object.

* The 2 meter telescope or Bernard Lyot Telescope ( used with a new generation stellar spectropolarimeter );

After his untimely early death from double pleurisy, his widow funded the Henry Draper Medal for outstanding contributions to astrophysics and a telescope, which was used to prepare the Henry Draper Catalog of stellar spectra.

During that period, the US Naval Observatory ( USNO ) relocated a meridian circle telescope to El Leoncito to extend their catalogue of stellar positions to the Southern Hemisphere.

His first undertaking at the Dublin Observatory was the erection of an equatorial telescope to carry the fine object-glass presented to the university by Sir James South ; and on its completion he began an important series of researches on stellar parallax.

Also installed were new instruments, such as the 65-cm ( 26-inch ) refractor, a horizontal meridian device, a photographic polar telescope, a big zenith telescope, stellar interferometer, 2 solar telescopes, coronagraph, a big radio telescope and all kinds of labware.

* Microvariability and Oscillations of STars telescope, a stellar photometric monitoring satellite built by Canada

In stellar aberration the position of a star when viewed with a telescope swings each side of a central position by about 20. 5 seconds of arc every six months.

In 1871 Airy demonstrated that stellar aberration occurs even when a telescope is filled with water.

It seems that if the aether drag hypothesis were true then stellar aberration would not occur because the light would be travelling in the aether which would be moving along with the telescope.

The asterism and its immediate surroundings are a useful gauge for determining the faintest stars visible in a small telescope as there are a wide range of stellar magnitudes within the cluster easily viewed in one small location of the sky.