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Lecture 2 Astronomical Distances
Lecture 2 Astronomical Distances

SPICA Yellow Book
SPICA Yellow Book

... and evolution occur. Deep exploration of the cold Universe using high spatial resolution observations in the Far Infrared (FIR) and sub-mm started in 2009 with the launch of the Herschel Space Observatory. Herschel is opening this almost unexplored window through photometric surveys of star formatio ...
Global star formation in the Milky Way from the VIALACTEA
Global star formation in the Milky Way from the VIALACTEA

Astro-MilkyWay
Astro-MilkyWay

... measurement of the distances to the globular clusters? a. The Sun is far from the center of the Milky Way. b. The Sun is near the center of the Milky Way. c. A period-luminosity relationship also exists for RR Lyrae variable stars. d. Globular clusters have 50,000 to 1,000,000 stars. e. Open cluster ...
The Milky Way
The Milky Way

... measurement of the distances to the globular clusters? a. The Sun is far from the center of the Milky Way. b. The Sun is near the center of the Milky Way. c. A period-luminosity relationship also exists for RR Lyrae variable stars. d. Globular clusters have 50,000 to 1,000,000 stars. e. Open cluster ...
Chapter 15
Chapter 15

Chapter 10
Chapter 10

Volcanoes and Igneous Activity Earth
Volcanoes and Igneous Activity Earth

... • Strong magnetic field • First one discovered in early 1970s • Pulsar (pulsating radio source) • Found in the Crab Nebula (remnant of an A.D. 1054 supernova) © 2011 Pearson Education, Inc. ...
Series Telescopes INSTRUCTION MANUAL
Series Telescopes INSTRUCTION MANUAL

... • All models can be used terrestrially as well as astronomically with the standard accessories included. Take time to read through this manual before embarking on your journey through the Universe. It may take a few observing sessions to become familiar with your telescope, so you should keep this m ...
Star
Star

... • Energy continues to be generated in the core of the star as hydrogen fuses into helium. • A star that has a mass about the same as the sun’s mass stays on the main sequence for about 10 billion years. • Scientists estimate that over a period of almost 5 billion years, the sun has converted only 5% ...
Cosmological Aspects of Nucleosynthesis
Cosmological Aspects of Nucleosynthesis

... 3 neutrino families More than 3 neutrino-families would have contributed to the mass density of ultrarelativistic particles. This would have speeded up the expansion in the radiationdominated universe. Neutrino would decouple at higher temperature and Helium ...
Teil 2
Teil 2

Evolution of the atomic and molecular gas content of galaxies
Evolution of the atomic and molecular gas content of galaxies

... gas and much lower cosmic H2 fraction over the entire redshift range probed than the pressure based recipe. These strong differences in Hi mass function and cosmic density between the two recipes are driven by low mass galaxies (log (M∗ /M⊙ ) 6 7) residing in low mass halos (log (Mvir /M⊙ ) 6 10). B ...
1. This question is about some of the properties of Barnard`s star
1. This question is about some of the properties of Barnard`s star

... This question is about some of the properties of Barnard’s star. Barnard’s star, in the constellation Ophiuchus, has a parallax angle of 0.549 arc-second as measured from Earth. (a) ...
First mapping of the area surrounding our solar system
First mapping of the area surrounding our solar system

Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... based on their light curves, that is, their pattern of rising and falling brightness. Later, they found these types actually corresponded to different physical circumstances triggering the explosions. Even those types have fine distinctions based on their spectra, giving rise to the categorization o ...
Chapter 17
Chapter 17

Resume
Resume

... During my PhD program at TIFR, I led the development, installation, calibration and upgrades of TIFR Near Infrared Spectrometer and Imager (TIRSPEC) at TIFR IR lab, which we installed on the side port of 2 meter Himalayan Chandra Telescope (HCT), Hanle, Ladakh, India. I developed various algorithms ...
Detection Technique for Artificially-Illuminated Objects in the Outer
Detection Technique for Artificially-Illuminated Objects in the Outer

... We first examine the feasibility of this new SETI technique within the Solar System, which offers the best prospects for detecting intrinsically faint sources of light. The flux reaching an observer from any self-luminous source varies according to the familiar inverse square law, but the flux from ...
Confirmation of Hostless Type Ia Supernovae Using Hubble Space
Confirmation of Hostless Type Ia Supernovae Using Hubble Space

... population is old (e.g. Sand et al. 2012). However, there is evidence that low levels of star formation are present in elliptical galaxies (e.g., Yi et al. 2005; Suh et al. 2011; Graham et al. 2012). Could it be that all SN Ia are actually from younger stellar populations? Probably not – for example ...
The Cosmic Microwave Background and the Big Bang Theory of the
The Cosmic Microwave Background and the Big Bang Theory of the

... dimension, which we 3-dimensional beings can visualize but is not part of the 2dimensional universe that is the surface of the balloon. As the balloon expands, the 2dimensional universe starts from a very small area and gets larger. But where is the center of the surface? It is NOT the center of the ...
THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting
THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting

CH01.AST1001.F16.EDS
CH01.AST1001.F16.EDS

- MNASSA Page
- MNASSA Page

... more than 30 arc minutes. It is a very nice object to study through binoculars. The Magellanic Cloud is home to NGC 2070, also known as Bennett 35, the great looped nebula situated in the south-eastern part of the Cloud and probably one of the most amazing objects in the southern night sky. Known as ...
CH01.AST1001.S15.EDS
CH01.AST1001.S15.EDS

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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.
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