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Spectroscopy: Unlocking the Secrets of Star Light
Spectroscopy: Unlocking the Secrets of Star Light

... temperature, how fast it is rotating and whether it is moving towards or away from us, how large and dense it is and what it is made of. Within the last decade planets beyond our Solar System have been discovered via their effect on the parent star's spectrum. Isaac Newton showed that a glass prism ...
12-1 - Piscataway High School
12-1 - Piscataway High School

... visual magnitude a star would have if it were 10 pc away as its absolute visual magnitude (MV). This is an expression of the intrinsic brightness of the star. The symbol for absolute visual magnitude is a capital M with a subscript V. The subscript reminds you it is a visual magnitude based only on ...
Spectroscopy: Unlocking the Secrets of Star Light
Spectroscopy: Unlocking the Secrets of Star Light

... temperature, how fast it is rotating and whether it is moving towards or away from us, how large and dense it is and what it is made of. Within the last decade planets beyond our Solar System have been discovered via their effect on the parent star's spectrum. Isaac Newton showed that a glass prism ...
Neutron star masses: dwarfs, giants and neighbors
Neutron star masses: dwarfs, giants and neighbors

... We consider the possible existence of a common channel of evolution of binary systems, which results in a GRB during the formation of a BH or the birth of a magnetar during the formation of a NS. We assume that the rapid rotation of the core of a collapsing star can be explained by tidal synchroniza ...
don_lamb  - New Views of the Universe
don_lamb - New Views of the Universe

...  Compact binary mergers  Merging compact objects (NS-NS or NS-BH)  Hypercritical accretion onto a newly formed black hole  Dominant timescale is set by accretion disk viscosity ...
Test 3 Review Clicker Questions
Test 3 Review Clicker Questions

... city blocks. c) two grains of sand 100 light- years apart. d) two golf balls 100 km apart. e) two baseballs 100 yards apart. ...
Fast Auto-Focus Method and Software for CCD
Fast Auto-Focus Method and Software for CCD

... 2. A full frame 3x3 binned image is taken with a minimal exposure time 3. The brightest star is found, the position determined and the HFD measured 4. The target star is sub-framed and a second exposure taken (download time is minimized due to the smaller frame size) 5. The focuser position is then ...
Fast Auto-Focus Method and Software for CCD-based
Fast Auto-Focus Method and Software for CCD-based

... 2. A full frame 3x3 binned image is taken with a minimal exposure time 3. The brightest star is found, the position determined and the HFD measured 4. The target star is sub-framed and a second exposure taken (download time is minimized due to the smaller frame size) 5. The focuser position is then ...
Science East Meteor Radiant Worksheet finished
Science East Meteor Radiant Worksheet finished

... Meteoroid: Dust and debris left behind from a comet or asteroid, floating in space (before it enters the atmosphere). These are small particles (no bigger than a boulder) anything bigger is called an asteroid. Meteors: Pieces of this dust or debris that enter the atmosphere and burns up. These are a ...
SherwoodWA_1973redux - Edinburgh Research Archive
SherwoodWA_1973redux - Edinburgh Research Archive

... 1970; Gottesman and Davis, 1970) found that the HII regions and blue supergiants (in associations) lie within the ...
a wide-field survey for variable stars
a wide-field survey for variable stars

... 1555/1554). Over 400 light-years away, at the edge of a molecular cloud, both star and nebula are seen to vary significantly in brightness but not necessarily at the same time, adding to the mystery of the intriguing region. T Tauri stars are now generally recognized as young (less than a few millio ...
Explosive sources of the highest energy radiation
Explosive sources of the highest energy radiation

... fields such as those found around pulsars. These conditions can be produced in a wide variety of astrophysical objects: from the Sun, to binary systems in our galaxy, to extragalactic objects such as gamma-ray bursts. ...
Milky Way Galaxy
Milky Way Galaxy

... The Universe is filled with these star systems which themselves cluster together into larger systems. ...
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Supernovae and Gamma-Ray Bursts (draft)

... current interest are briefly discussed. ...
Betelgeuse - TeacherWeb
Betelgeuse - TeacherWeb

... Betelgeuse, called Alpha Orionis, is a star that makes up Orion’s shoulder in the east. It is 430 light years away from our solar system! It still shines bright in our sky at a magnitude of 0.5. Magnitude being the brightness of a star or celstial being. ...
Starry Night Companion - Starry Night Education
Starry Night Companion - Starry Night Education

Stars & Galaxies - newmanlib.ibri.org
Stars & Galaxies - newmanlib.ibri.org

... Galaxy Types • Galaxies are usually categorized by shape into three types: – Elliptical – Spiral – Irregular ...
The Nature of the Stars
The Nature of the Stars

Neon abundances - UCL Astrophysics Group
Neon abundances - UCL Astrophysics Group

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The old globular cluster system of the dIrr galaxy NGC 1427A in the

... level. Lower thresholds were found to give too many spurious detections. Visual image inspection showed that no objects were missed and only few false detections were included in the lists. In order to improve the faint object photometry the underlying and extended galaxy light was subtracted form t ...
1 Pau Amaro Seoane - modest 15-s
1 Pau Amaro Seoane - modest 15-s

... of turbulent molecular clouds. The stars are assumed to form in the densest regions in the collapsing cloud after an initial free-fall times of the molecular cloud. The dynamical evolution of these stellar distributions are continued by means of direct N-body simulations. The molecular clouds typica ...
Multiwavelength properties of γ-ray loud binary systems.
Multiwavelength properties of γ-ray loud binary systems.

... of -ray-loud binaries. In this respect, it is not surprising that the highest excess variability is found in the directions of known γ-ray-loud binary systems: LSI +61 303, V407 Cyg, Cyg X-3 and PSR B1259-63. Remarkably, there are no signatures of weaker variability which could be clearly associated ...
Supernovae - University of Texas Astronomy Home Page
Supernovae - University of Texas Astronomy Home Page

... heavens favored Kepler in his turn with the explosion of a supernova in 1604. Kepler also took careful data by which we deduce that he witnessed the same kind of explosion as his master. Although there are counterarguments and some controversy, both Tycho's and Kepler's supernovae are widely regard ...
Effect of the stellar spin history on the tidal evolution of close
Effect of the stellar spin history on the tidal evolution of close

... Methods. We used a standard equilibrium tidal model to compute the orbital evolution of single planets orbiting both Sun-like stars and very low-mass stars (0.1 M ). We tested two stellar spin evolution profiles, one with fast initial rotation (1.2 day rotation period) and one with slow initial rot ...
Dust and molecular gas in the most distant quasars
Dust and molecular gas in the most distant quasars

... detections show FIR excesses in their SEDs. • The MAMBO undetected quasars at z~6: – The average FIR-to-radio SED is consistent with the templates of local optical quasars. – The average FIR to AGN-bolometric luminosity ratio follows the trend defined by local PG quasars. ...
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Cygnus (constellation)



Cygnus /ˈsɪɡnəs/ is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan. The swan is one of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross (in contrast to the Southern Cross). Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.Cygnus contains Deneb, one of the brightest stars in the night sky and one corner of the Summer Triangle, as well as some notable X-ray sources and the giant stellar association of Cygnus OB2. One of the stars of this association, NML Cygni, is one of the largest stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion that was the first object widely held to be a black hole. Many star systems in Cygnus have known planets as a result of the Kepler Mission observing one patch of the sky, the patch is the area around Cygnus. In addition, most of the eastern part of Cygnus is dominated by the Hercules–Corona Borealis Great Wall, a giant galaxy filament that is the largest known structure in the observable universe; covering most of the northern sky.
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