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NEW QUESTION: 1
You are making selection by using the elliptical marquee. The value for Feather is set 10 pixels. When would you see the effect of the feathering option?
A. When you move the selected pixels
B. As soon as you finish making the selection
C. When you choose Select>Feather
D. When you deselect
Answer: A

NEW QUESTION: 2
What statement about 802.3, Clause 33 Power over Ethernet is true?
A. The lowest voltage drop is achieved when using CAT6 cable instead of Cat5 or CAT5e.
B. Only endpoint PSEs are supported.
C. Only midspan PSEs are supported.
D. When using CAT5 cabling, you increase the maximum draw available to the PD over that available with CAT6.
Answer: A
Explanation:
https://www.cablinginstall.com/articles/2012/08/cat-6a-vs-cat-5e-poe.html

NEW QUESTION: 3
Refer to the exhibit.

Which two options provide the best loop protection in this topology, regardless of a bridged domain configuration? (Choose two.)
A. REP on all switches
B. BPDU guard on Switch A and Switch D
C. MST on all switches
D. 8032 on ring A-B-C-D
E. PVRSTP on all switches
Answer: A,D

NEW QUESTION: 4
The discoveries of the white dwarf, the neutron star, and the black hole, coming well after the discovery of the red giant are among eh most exciting developments in decades because they may be well present physicists with their greatest challenge since the failure of classical mechanics. In the life cycle of the star, after all of the hydrogen and helium fuel has been burned, the delicate balance between the outer nuclear radiations. Pressure and the stable gravitational force becomes disturbed and slow contraction begins. As compression increases, a very dense plasma forms. If the initial star had mass of less than 1.4 solar masses (1.4 times the mass of our sun), the process ceases at the density of 1,000 tons per cubic inch, and the star becomes the white dwarf. However, if the star was originally more massive, the white dwarf plasma can't resist the gravitations pressures, and in rapid collapse, all nuclei of the star are converted to a gas of free neutrons. Gravitational attraction compresses this neutron gas rapidly until a density of 10 tons per cubic inch is reached; at this point the strong nuclear force resists further contraction. If the mass of the star was between 1.4 and a few solar masses, the process stops here, and we have a neutron star. But if the original star was more massive than a few solar masses, even the strong nuclear forces cannot resist the gravitational brunch. The neutrons are forced into one another to form heavier hadrons and these in turn coalesce to form heavier entities, of which we as yet know nothing. At this point, a complete collapse of the stellar mass occurs; existing theories predict a collapse to infinite density and infinitely small dimensions Well before this, however, the surface gravitational force would become so strong that no signal could ever leave the star - any photon emitted would fall back under gravitational attraction - and the star would become black hole in space. This gravitational collapse poses a fundamental challenge to physics. When the most widely accepted theories predict such improbable things as infinite density and infinitely small dimensions, it simply means that we are missing some vital insight. This last happened in physics in the 1930's, when we faced the fundamental paradox concerning atomic structure. At that time, it was recognized that electrons moved in table orbits about nuclei in atoms. However, it was also recognized that if charge is accelerated, as it must be to remain in orbit, it radiates energy; so, theoretically, the electron would be expected eventually to spiral into the nucleus and destroy the atom.
Studies centered around this paradox led to the development of quantum mechanics. It may well be that an equivalent t advance awaits us in investigating the theoretical problems presented by the phenomenon of gravitational collapse.
The author asserts that the discoveries of the white dwarf, the neutron star, and the black hole are significant because these discoveries.
A. establish the relationship between the mass and gravitational pressure.
B. demonstrate the probability of infinite density and infinitely small dimensions.
C. pose the most comprehensive and fundamental problem faced by physicists in decades.
D. assist in establishing the age of the universe by tracing the life histories of stars.
E. clarify the paradox suggested by the collapse of electrons into atomic nuclei.
Answer: C
Explanation:
Explanation/Reference:
Explanation:

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