A) shock waves from explosive star formation in the nuclear bulge
B) density waves in the interstellar medium
C) satellite galaxies plunging through the disk of the nuclear spiral galaxy
D) self-propagating star formation, where star formation occurs in bursts
Correct Answer
verified
Multiple Choice
A) H0 * recessional speed = distance.
B) recessional speed = H0 *distance.
C) recessional speed = H0, which is constant.
D) recessional speed * distance = H0.
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verified
Multiple Choice
A) the proton and electron in hydrogen.
B) the planets and the Sun.
C) galaxies in the Local Group.
D) superclusters of galaxies.
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verified
Multiple Choice
A) poor regular
B) poor irregular
C) rich regular
D) rich irregular
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Multiple Choice
A) the spiral arms in these galaxies are strongly influenced by the black hole at the center of the galaxy.
B) the density wave has been disrupted by the bar across the center of the galaxy.
C) dust lanes occur in broad bands rather than in the narrow bands found in grand-design spirals.
D) the spiral arm segments are defined only by the relatively short-lived O- and B-type stars.
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verified
Multiple Choice
A) SBa
B) Sc
C) Sb
D) Sa
Correct Answer
verified
Multiple Choice
A) equivalent of a massive "sound" wave generated at the center of the galaxy by the gravitational energy release at the initial formation of the galaxy, producing progressive compression of material that is shaped by galaxy rotation
B) gravitational influence from the rotating central supermassive black hole at the galactic center of the arm material
C) gravitational interaction from the close passage of another galaxy
D) shock waves from supernova explosions of massive stars within the spiral arms
Correct Answer
verified
Multiple Choice
A) primarily young, metal-rich stars
B) stars of all ages, but all metal-poor
C) primarily old, metal-poor stars
D) stars of all ages from young, metal-rich stars to old, metal-poor stars
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verified
Multiple Choice
A) large numbers of cool, dark, brown dwarf stars floating in the galaxy cluster
B) very hot intergalactic gas emitting X-rays in clusters.
C) a tremendous flux of neutrinos, which have recently been shown to have mass, coming from these clusters.
D) large numbers of small but massive black holes within every galaxy.
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verified
Multiple Choice
A) is probably type Sa.
B) is probably type Sb.
C) is probably type Sc.
D) cannot be classified if its spiral arms cannot be studied.
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verified
Multiple Choice
A) Sb
B) SBb
C) Sa
D) Sc
Correct Answer
verified
Multiple Choice
A) only over distances about the size of a galaxy or larger; consequently, the Milky Way Galaxy expands, but the solar system does not.
B) only between objects separated by a vacuum; as a result, the bodies do not expand, but the Earth-Moon system does.
C) between all objects, even between the atoms in the bodies, although the expansion of a person is too small to be measured reliably.
D) primarily in the huge voids between clusters of galaxies. "Small" objects like galaxies or Earth do not expand.
Correct Answer
verified
Multiple Choice
A) Sa
B) SBb
C) Sc
D) Sb
Correct Answer
verified
Multiple Choice
A) The observed mass of the galaxies of the cluster is many thousands of times too small to hold the cluster together.
B) The observed mass of the galaxies of the cluster is about 10 times larger than the amount needed to hold the cluster together.
C) The observed mass of the galaxies in the cluster is about 10 times too small to hold the cluster together.
D) The observed mass of the galaxies of the cluster is almost exactly equal to the mass needed to hold the cluster together.
Correct Answer
verified
Multiple Choice
A) hot interstellar gas, detected by recent space-borne X-ray telescopes
B) concentration of galaxies into clusters and superclusters
C) distorted spiral arms in many galaxies
D) initiation of significant new star formation in so-called starburst galaxies
Correct Answer
verified
Multiple Choice
A) 970 million ly
B) 6.7 billion ly
C) 13.4 billion ly
D) 56 billion ly
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verified
Multiple Choice
A) irregular galaxies
B) barred spirals
C) large spirals
D) ellipticals
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verified
Multiple Choice
A) The winding dilemma is the basic cause of the chaotic structure in flocculent spirals.
B) The winding dilemma affects only galaxies with flat rotation curves and constant stellar speeds, and this does not include flocculent spirals.
C) Flocculent spirals are dominated by self-propagating star formation in which groups of stars are formed and then fade as the massive luminous stars complete their life cycles. This transient, spotty star-formation pattern is unaffected by the winding dilemma.
D) Flocculent spirals have a whirlpool structure with several centers of rotation, each affected by the winding dilemma. This results in the overall flocculent pattern.
Correct Answer
verified
Multiple Choice
A) Superclusters are distributed more or less evenly (i.e., at random) throughout the universe.
B) Superclusters are distributed in long lines that cover the universe like a gigantic fishing net.
C) Superclusters are separated by large voids, appearing at the intersection of filaments.
D) Superclusters are grouped into clusters of superclusters that in turn are grouped into clusters of clusters, and so on.
Correct Answer
verified
Multiple Choice
A) X-ray
B) visible
C) infrared
D) radio
Correct Answer
verified
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