
Galaxy Evolution
... Fig. 2.—Top: Determination of cluster and group baryon fractions within r500 as a function of M500 (bottom axis) and velocity dispersion (top axis). X-ray gas mass fractions from Vikhlinin et al. (2006; circles) and Gastaldello et al. (2006; triangles) and the stellar mass fractions ( BCG +ICL+galax ...
... Fig. 2.—Top: Determination of cluster and group baryon fractions within r500 as a function of M500 (bottom axis) and velocity dispersion (top axis). X-ray gas mass fractions from Vikhlinin et al. (2006; circles) and Gastaldello et al. (2006; triangles) and the stellar mass fractions ( BCG +ICL+galax ...
Document
... as a framework for how that history made our existence possible. So first we need to know something of the structure and arrangement of this universe whose history we want to describe. Theme - Gaining perspective on how we connect to the universe: we are products of the whole universe, not just our ...
... as a framework for how that history made our existence possible. So first we need to know something of the structure and arrangement of this universe whose history we want to describe. Theme - Gaining perspective on how we connect to the universe: we are products of the whole universe, not just our ...
word document - FacStaff Home Page for CBU
... *8. Does the sun actually rise earlier or later than it appears to? What causes this? *9. How does the atmosphere affect light from astronomical bodies? Give one example for each of the three major ways. *10. What are the Van Allen radiation belts? 11. Because of the earth's rotation about its axis, ...
... *8. Does the sun actually rise earlier or later than it appears to? What causes this? *9. How does the atmosphere affect light from astronomical bodies? Give one example for each of the three major ways. *10. What are the Van Allen radiation belts? 11. Because of the earth's rotation about its axis, ...
Galaxy / Cluster Ecosystem Ming Sun (University of Alabama in Huntsville)
... rotation pattern and suggests turbulence not strong (Sun + 2006, 2007, 2010) ...
... rotation pattern and suggests turbulence not strong (Sun + 2006, 2007, 2010) ...
Probing the Atmospheres of Exoplanets
... external solar systems has been truly remarkable. (Note: both “exoplanet” and “extrasolar planet” are used interchangeably in this article.) By early 2009, more than 340 planets had been found orbiting other stars—almost all of them discovered indirectly by ground-based telescopes as a result of the ...
... external solar systems has been truly remarkable. (Note: both “exoplanet” and “extrasolar planet” are used interchangeably in this article.) By early 2009, more than 340 planets had been found orbiting other stars—almost all of them discovered indirectly by ground-based telescopes as a result of the ...
the rest of the univ..
... It is estimated that there are at least 35,000 Kuiper Belt objects greater than 100 km in diameter, which is several hundred times the number (and mass) of similar sized objects in the main asteroid belt. A team of astronomers led by Anita Cochran report that the Hubble Space Telescope has detected ...
... It is estimated that there are at least 35,000 Kuiper Belt objects greater than 100 km in diameter, which is several hundred times the number (and mass) of similar sized objects in the main asteroid belt. A team of astronomers led by Anita Cochran report that the Hubble Space Telescope has detected ...
Light, spectra, Doppler shifts
... iron hydride (FeH) and methane (CH4) in their spectra. These are very cool stars, detectable at infrared wavelengths only. ...
... iron hydride (FeH) and methane (CH4) in their spectra. These are very cool stars, detectable at infrared wavelengths only. ...
Light, spectra, Doppler shifts
... iron hydride (FeH) and methane (CH4) in their spectra. These are very cool stars, detectable at infrared wavelengths only. ...
... iron hydride (FeH) and methane (CH4) in their spectra. These are very cool stars, detectable at infrared wavelengths only. ...
Standard candles
... white dwarf star in a binary pair with a red dwarf star steals mass from the red dwarf until it is too massive to support itself against gravity any more. Then its core collapses, starting a runaway nuclear reaction and a bright explosion. Because the collapse always happens at the same mass, the lu ...
... white dwarf star in a binary pair with a red dwarf star steals mass from the red dwarf until it is too massive to support itself against gravity any more. Then its core collapses, starting a runaway nuclear reaction and a bright explosion. Because the collapse always happens at the same mass, the lu ...
Competitive advantage
... HECTOR: Bottom Line › Spectral resolution is extremely important for this science. › Ideal: R=7000 both red (i.e. @ 6500A) and blue (i.e. @ 4500A) › Minimal: R=5000 in Red and R=3000 in blue: Red line in Robert’s 4x 2kx 2k resolution vs λ plot would work, among others. ...
... HECTOR: Bottom Line › Spectral resolution is extremely important for this science. › Ideal: R=7000 both red (i.e. @ 6500A) and blue (i.e. @ 4500A) › Minimal: R=5000 in Red and R=3000 in blue: Red line in Robert’s 4x 2kx 2k resolution vs λ plot would work, among others. ...
Cartwheel Galaxy - Chandra X
... Galaxy was probably a normal spiral structure galaxy similar to the Milky Way Galaxy before the collision. The spiral structure is beginning to re-emerge, as seen in the faint arms or spokes between the outer ring and the bulls-eye shaped nucleus. The gravitational disruption of a smaller intruder g ...
... Galaxy was probably a normal spiral structure galaxy similar to the Milky Way Galaxy before the collision. The spiral structure is beginning to re-emerge, as seen in the faint arms or spokes between the outer ring and the bulls-eye shaped nucleus. The gravitational disruption of a smaller intruder g ...
Finnish Centre for Astronomy with ESO
... in astronomical research. The ultimate goal of FINCA is to improve the scientific and industrial benefit of Finland’s membership in ESO, and Finland’s international competitiveness in astronomical research. The year 2014 marked the 5th year of operation for FINCA, administratively a Special Unit of ...
... in astronomical research. The ultimate goal of FINCA is to improve the scientific and industrial benefit of Finland’s membership in ESO, and Finland’s international competitiveness in astronomical research. The year 2014 marked the 5th year of operation for FINCA, administratively a Special Unit of ...
F P US R
... "The committee will solicit input from the community at large. Its goal is to publish a ‘white paper’, which will be relevant for the broad astronomy community and timely for the planning of the next Decadal Survey." The committee members were selected by Dr. Schreier after extensive consultation wi ...
... "The committee will solicit input from the community at large. Its goal is to publish a ‘white paper’, which will be relevant for the broad astronomy community and timely for the planning of the next Decadal Survey." The committee members were selected by Dr. Schreier after extensive consultation wi ...
File
... brick and cement (this is why you can get radio reception almost anywhere). Radio waves can also be picked up during the day so scientists can work at any time (optical telescopes can only be used at night.) Having such large waves requires a large object to read these waves. To the right is a radio ...
... brick and cement (this is why you can get radio reception almost anywhere). Radio waves can also be picked up during the day so scientists can work at any time (optical telescopes can only be used at night.) Having such large waves requires a large object to read these waves. To the right is a radio ...
Hubble Deep Field

The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area 2.5 arcminutes across, about one 24-millionth of the whole sky, which is equivalent in angular size to a 65 mm tennis ball at a distance of 100 metres. The image was assembled from 342 separate exposures taken with the Space Telescope's Wide Field and Planetary Camera 2 over ten consecutive days between December 18 and December 28, 1995.The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all of the 3,000 objects in the image are galaxies, some of which are among the youngest and most distant known. By revealing such large numbers of very young galaxies, the HDF has become a landmark image in the study of the early universe, with the associated scientific paper having received over 900 citations by the end of 2014.Three years after the HDF observations were taken, a region in the south celestial hemisphere was imaged in a similar way and named the Hubble Deep Field South. The similarities between the two regions strengthened the belief that the universe is uniform over large scales and that the Earth occupies a typical region in the Universe (the cosmological principle). A wider but shallower survey was also made as part of the Great Observatories Origins Deep Survey. In 2004 a deeper image, known as the Hubble Ultra-Deep Field (HUDF), was constructed from a few months of light exposure. The HUDF image was at the time the most sensitive astronomical image ever made at visible wavelengths, and it remained so until the Hubble Extreme Deep Field (XDF) was released in 2012.