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Page "Nucleosynthesis" ¶ 23
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Gamma and ray
Legend: γ = Gamma ray s HX = Hard X-ray s SX = Soft X-Rays EUV = Extreme-ultraviolet NUV = Near-ultraviolet Visible light ( colored bands ) NIR = Near-infrared MIR = Moderate-infrared FIR = Far-infrared EHF = Extremely high frequency ( microwaves ) SHF = Super-high frequency ( microwaves ) UHF = Ultrahigh frequency ( radio waves ) VHF = Very high frequency ( radio ) HF = High frequency ( radio ) MF = Medium frequency ( radio ) LF = Low frequency ( radio ) VLF = Very low frequency ( radio ) VF = Voice frequency ULF = Ultra-low frequency ( radio ) SLF = Super-low frequency ( radio ) ELF = Extremely low frequency ( radio )
* Gamma ray
A Gamma ray burst ( GRB ) found in conjunction with a supernova has been called a Rosetta Stone for understanding the origin of GRBs.
Astronomical objects commonly studied in this field may include black holes, neutron stars, active galactic nuclei, supernovae, supernova remnants, and Gamma ray bursts.
Gamma ray bursts are the most powerful explosions that occur in the universe.
Gamma ray bursts are not rare events.
* Gamma ray burst
* 2004-- Success-Launch of the Swift Gamma ray burst observatory.
* Gamma ray spectrometer, an instrument for detecting elements
* Gamma ray burster
Gamma perforators operate in much the same way as an open hole natural gamma ray tool.
The Rosemary Hill Observatory ( RHO ) started observing 3C 279 in 1971, and was further observed by the Compton Gamma Ray Observatory in 1991, when it was unexpectedly discovered to be one of the brightest gamma ray objects in the sky.
Five months after deployment, NASA renamed the satellite the Arthur Holly Compton Gamma Ray Observatory, or Compton Observatory, after the Nobel Prize-winning physicist who did important work in gamma ray astronomy.
This mission was launched on April 5, 1991, and featured the deployment of the Gamma Ray Observatory for the purpose of exploring gamma ray sources throughout the universe.
Grunsfeld studied binary pulsars and energetic x-ray and gamma ray sources using the NASA Compton Gamma Ray Observatory, x-ray astronomy satellites, radio telescopes, and optical telescopes including the NASA Hubble Space Telescope.
During the 93 orbits of the mission, the crew deployed the Gamma Ray Observatory ( GRO ) to study gamma ray sources in the universe.
* Gamma ray spectrometer-GS-12V
* Gamma ray densitometer-RP-75
* Gamma ray spectrometer-GS-12V
* Gamma ray densitometer-RP-75
Gamma rays striking the bismuth atoms produced a flash of light with an intensity proportional to the energy of the gamma ray which was recorded by detectors.
His leadership of the Compton Gamma Ray Observatory and the Swift Mission has led to new insights into the extreme physics of active galactic nuclei and gamma ray bursts ".
During this mission the crew aboard the Shuttle Atlantis deployed the Gamma Ray Observatory ( GRO ) for the purpose of exploring gamma ray sources throughout the universe, and conducted the first scheduled space walk in more than five and one-half years.
See Gamma ray detector

Gamma and lines
Audi, Volkswagen, Porsche, Mercedes, Vauxhall, Pontiac and BMW all fit Blaupunkt products into their cars, often branded with the car manufacturer's own mark ( e. g. The VW Gamma or Audi Symphony lines ), with Fiat using them, occasionally unbranded but generally unmodified.
Gamma rays, emitted from the nuclei of atoms, show up as sharp emission lines on the instrument's spectrum output.
Gamma Ursae Majoris is an Ae star, which is surrounded by an envelope of gas that is adding emission lines to the spectrum of the star ; hence the ' e ' suffix in the stellar classification of A0 Ve.

Gamma and <
( The ACT concept is drawn from the Marvel Super Heroes game published by TSR shortly before development of Gamma World < nowiki >'</ nowiki > s third edition.
Gamma World < nowiki >'</ nowiki > s fourth edition abandoned the Action Control Table in favor of mechanics derived from the Advanced Dungeons & Dragons 2nd Edition rules, although some mechanics presage Alternity and the 3rd edition D & D rules.
Gamma ( γ ) radiation consists of photons with a frequency of greater than 10 < sup > 19 </ sup > Hz.
Upper part: Gamma Orionis, Algol | Algol B, the Sun ( centre ), underneath their darker mirror images < span style =" white-space: nowrap ;">( artist's interpretation ),</ span > and < span style =" white-space: nowrap ;"> 1 E8 m | other objects ,</ span > to scale.
Gamma rays would Compton scatter in a forward detector module, where the interaction energy E < sub > 1 </ sub >, given to the recoil electron was measured, while the Compton scattered photon would then be caught in one of a second layer of scintillators to the rear, where its total energy, E < sub > 2 </ sub >, would be measured.
* 1. 4 * 10 < sup > 33 </ sup > m³ = volume of Gamma Crucis, a red giant in Crux
F. G. Kenyon — Gamma ( γ )< ref name = Kenyon > Frederic G. Kenyon, " Handbook to the Textual Criticism of the New Testament ", London < sup > 2 </ sup >, 1912, pp. 334-338 .</ ref >
* Pi Gamma Mu ( ΠΓΜ ) – 1924 ; co-ed social sciences honor society < nowiki >*</ nowiki >
It is a suspected Gamma Cassiopeiae type ( GCAS ) variable star, with its apparent magnitude varying from 2. 62 < sup > m </ sup > to 2. 66 < sup > m </ sup >.
The Lanczos approximation was popularized by Numerical Recipes, according to which computing the Gamma function becomes " not much more difficult than other built-in functions that we take for granted, such as sin x or e < sup > x </ sup >".
Gamma ray spectroscopy has indicated that < sup > 229 </ sup > Th has a nuclear isomer with a remarkably low excitation energy.
Most stars of this type are slow rotators, but Gamma Trianguli Australis displays a very high rate of rotation with a projected rotational velocity of 199 km s < sup >– 1 </ sup >.

Gamma and >
These generalised functions can equivalently be expressed for x > 0 using the Gamma function and incomplete Gamma function:

Gamma and 56
Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3. 65 and 3. 56, and of spectral type F0V.

0.432 seconds.