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PPT Only - Harvard-Smithsonian Center for Astrophysics
PPT Only - Harvard-Smithsonian Center for Astrophysics

... highlights the extreme depletion seen at high extinctions in C18O emission (Lada et al. 2001). The inset on the bottom right panel shows the extinction map derived from applying the NICER method applied to NTT near-infrared observations of the most extinguished portion of B68. The graph in the botto ...
NAS biographical memoir of Martin Schwarzschild
NAS biographical memoir of Martin Schwarzschild

... Background and early years in Europe Nature and nurture conspired to provide an ideal scientific environment for Martin Schwarzschild, but the early years must have been difficult. He was born to a distinguished and assimilated German-Jewish family in 1912—two years before the outbreak of World War ...
Astro Review - Parkway C-2
Astro Review - Parkway C-2

... 67. Which stars are composed of matter in which electrons have combined with protons? 68. A comet’s tail always points ____. 69. The measure of a star’s brightness is called its ____. 70. The sun can continue to exist in its present stable state for about another ____. 71. By observing sunspots, Ga ...
are coronae of late-type stars made of solar-like structures? the x
are coronae of late-type stars made of solar-like structures? the x

... overall trend suggests that the confined plasma in the corona of a late-type star, on the average, gets brighter as it gets hotter. Analogously, Marino et al. (2002b) reported the data of 40 late-type stars of spectral type between F7 and K2 within 25 pc from the Sun in an analogous FX versus HR dia ...
Tycho Brahe
Tycho Brahe

... even though he was not the 1st to discover it. (The SNR remnant is visible as a nebula) ...
Cosmic variance in [O/Fe] in the Galactic disk
Cosmic variance in [O/Fe] in the Galactic disk

Galaxies
Galaxies

... Galaxy mass measurements show that galaxies need between 3 and 10 times more mass than can be observed to explain their rotation curves. The discrepancy is even larger in galaxy clusters, which need 10 to 100 times more mass. The total needed is more than the sum of the dark matter associated with e ...
A Search for Extrasolar Planets Using Echoes Produced in Flare
A Search for Extrasolar Planets Using Echoes Produced in Flare

... The variable nature of stars has a long documented history. In any portion of the sky, stars can be found in various states from quiescence to obliteration. Of the myriad of observable characteristics on either short or long timescales compared to a human lifetime, a particular type of short-term va ...
2012 NSS Phy 2-(E).
2012 NSS Phy 2-(E).

hwd_ewd_v3 - X-ray and Observational Astronomy Group
hwd_ewd_v3 - X-ray and Observational Astronomy Group

... The basis for understanding the nature of most stars is analysis of their optical spectra and classification according to the characteristics revealed. A number of physical processes can alter the atmospheric composition of a white dwarf as it cools. As noted by Schatzman4, the strong gravitational ...
Planetesimal collisions in binary systems
Planetesimal collisions in binary systems

... roughly solar mass of both stellar components make the system a prime target for finding an Earth mass planet in the habitable zone (Guedes et al. 2008). However, the α Centauri system is more extreme than γ Cephei with a mass ratio close to one (MA? = 1.1 M and MB? = 0.93 M ), eb = 0.52, and ab = ...
A Spectroscopic Survey of a Sample of Active M Dwarfs.
A Spectroscopic Survey of a Sample of Active M Dwarfs.

... to see whether their X-ray brightness indicated strong chromospheric activity: what fraction of Fleming’s stars are dMe stars? Fleming (1998) had shown that these stars probably have small proper motions, so we were interested in seeing whether other indications of youth are present. It has long bee ...
Imaging Uranus
Imaging Uranus

... indeed it has been suggested that Miranda was once a larger body which was broken up by an impact with another body and then re-formed. Of course no one can be certain, but given Uranus’ peculiar orbital inclination, and the geological structure of the surfaces of its satellites, it seems that the p ...
Nucleosynthesis and Chemical Evolution of Oxygen
Nucleosynthesis and Chemical Evolution of Oxygen

An Unbiased Near-infrared Interferometric Survey for Hot
An Unbiased Near-infrared Interferometric Survey for Hot

... evolution of extrasolar planetary systems. However, debris discs that are relatively easy to detect are located several astronomical units (au) to a few hundreds of au from their host stars, and thus only trace the outer regions of planetary systems. In order to study the inner regions close to the ...
Abstracts - Physics of Evolved Stars 2015
Abstracts - Physics of Evolved Stars 2015

Astronomy, Astrophysics, and Cosmology
Astronomy, Astrophysics, and Cosmology

Are there 12 or 13 Zodiac Signs?
Are there 12 or 13 Zodiac Signs?

... News of this supposedly 13-sign zodiac quickly travelled across the world, being featured (on the strength of the BBC's reputation) on NBC news in the US, and making countless sensational newspaper headlines throughout Europe, Canada, Brazil and Australia. Investigation into the source of the story ...
Understanding the zodiac, and why there really are 12 signs of the
Understanding the zodiac, and why there really are 12 signs of the

... News of this supposedly 13-sign zodiac quickly travelled across the world, being featured (on the strength of the BBC's reputation) on NBC news in the US, and making countless sensational newspaper headlines throughout Europe, Canada, Brazil and Australia. Investigation into the source of the story ...
File
File

Lecture21 - Michigan State University
Lecture21 - Michigan State University

... towards us • These measurements were announced in 1914, years before Hubble found that these spiral nebula were galaxies and before anyone knew how far away they were ISP 205 - Astronomy Gary D. Westfall ...
Document
Document

... Springel et al. 2005 ...
Stellar Spectroscopy
Stellar Spectroscopy

... For example, most of the stars are from the Henry Draper catalog of bright stars, and are given an “hd” prefix. The names of some of the other stars indicate their location; e.g., “EQ Peg” is located in the constellaction of Pegasus. Spectra of the Messier objects M74, a globular cluster, and M76, t ...
No. 6
No. 6

... the constellation of Ophiuchus. The star should disappear for up to 3 seconds maximum. The towns of Ahwaz and Abadeh (see figure 1) are in the predicted path but the error is nearly 1 full path width in both directions. Luckily there are no moon issues and the target star is located (as seen from Ah ...
Disentangling degenerate solutions from primary transit and
Disentangling degenerate solutions from primary transit and

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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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