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Gas cloud forming into a galaxy
In physical cosmology, a protogalaxy, which could also be called a "primeval galaxy", is a cloud of gas which is forming into a galaxy. It is believed
Protogalaxy
2010 video game
ProtoGalaxy is a cross-genre video game for Microsoft Windows that was released on October 6, 2010. In the game's back-story, a species of powerful, unknown
ProtoGalaxy
System of stars and interstellar matter
halos. These primordial structures allowed gasses to condense in to protogalaxies, large scale gas clouds that were precursors to the first galaxies.
Galaxy
Hypothetical invisible cosmic material
to form a dwarf galaxy. This collection of mass is sometimes called a protogalaxy. Dark matter particles are classified as cold, warm, or hot if their
Dark_matter
Natural physical entity in space
Ring Irregular By size Brightest cluster Giant elliptical Dwarf By type Protogalaxy Starburst Dark Active Radio Seyfert Quasar Microquasar Blazar BL Lac
Astronomical_object
Physical theory of the cosmos
galaxies in the foreground plane – nearly mature galaxies from 5 to 9 billion years ago – protogalaxies, blazing with young stars, beyond 9 billion years.
Big_Bang
Galaxy filament
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Coma_Filament
NASA satellite of the Explorer program
and 9-15 μm, specifically focusing on starburst galaxies and luminous protogalaxies. WIRE had problems and was unable to carry out its IR survey, and was
Wide_Field_Infrared_Explorer
Type of starburst galaxy
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Blueberry_galaxy
Trace radiation from the early universe
Robert (December 1967). "Thermal Cosmic Radiation and the Formation of Protogalaxies". Proceedings of the National Academy of Sciences. 58 (6): 2179–2186
Cosmic_microwave_background
[citation needed] October 6 Cut the Rope iOS [citation needed] October 6 ProtoGalaxy WIN [citation needed] October 7 Kingdom Hearts Re:coded DS [citation
2010_in_video_games
Large gas cloud in the constellation Cetus
miles (122×1021 kilometers). This nebular gas cloud is thought to be a protogalaxy, caught in the act of formation. There have been no spectroscopic signatures
Himiko_(Lyman-alpha_blob)
Galaxy with a high luminosity
"A high-redshift IRAS galaxy with huge luminosity—hidden quasar or protogalaxy?". Nature. 351 (6329): 719–721. Bibcode:1991Natur.351..719R. doi:10.1038/351719a0
Luminous_infrared_galaxy
protocluster found and spectroscopically confirmed to date. Galaxy or protogalaxy MoM-z14 z = 14.4 Quasar UHZ1 z ≅ 10.0 Black hole GN-z11 z = 10.6034±0
List of the most distant astronomical objects
List_of_the_most_distant_astronomical_objects
Deep-field space image in Fornax
foreground plane, nearly mature galaxies from 5 to 9 billion years ago, and protogalaxies beyond 9 billion years. Video (02:42) about how the Hubble eXtreme Deep
Hubble_Ultra-Deep_Field
3rd-century Queen of Yamataikoku
Lyman-alpha blob (a massive concentration of hydrogen gas believed to be a protogalaxy) that was discovered in 2009. Massing close to 40 billion suns and located
Himiko
Galaxy protocluster in the constellation Fornax
JWST Advanced Deep Extragalactic Survey (JADES). Farthest protoclusters Protogalaxy "NASA Telescopes Spot Surprisingly Mature Cluster in Early Universe |
JADES-ID1
One of the most distant quasars known
embedded in a protogalaxy in the midst of forming, and possibly creating the first Population III stars for the galaxy, or a pre-protogalaxy core still embedded
ULAS_J1120+0641
Astrophysics observatory in southern India
astrophysical phenomena such as pulsars, solar wind, recombination lines, and protogalaxies. As of 2017[update], the ORT is undergoing a major upgrade to its receiver
Ooty_Radio_Telescope
Galaxy filament containing the Perseus-Pisces Supercluster
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Perseus–Pegasus_Filament
Galaxy in the constellation Ursa Major
(comoving distance) Apparent magnitude (V) 29.6U Characteristics Type Protogalaxy Mass 1×1011 M☉ Size 1.8 kpc (5.9 kly) Other designations Sparky, GOODS-N-774
GOODS-N-774
Accumulation of particles into a massive object by gravitationally attracting more matter
enough kinetic energy, and dark matter coalesced sufficiently, to form protogalaxies. As further accretion occurred, galaxies formed. Indirect evidence is
Accretion_(astrophysics)
Galaxy that orbits a larger galaxy due to gravitational attraction
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Satellite_galaxy
Constellation in the southern celestial hemisphere
about 120 light-years (37 pc) across. UDFj-39546284 is a candidate protogalaxy located in Fornax, although recent analyses have suggested it is likely
Fornax
New Zealand astronomer (1941–1981)
closed or open. Her galaxy models led to the first approximation of what protogalaxies should look like. In 1974 she received the American Astronomical Society's
Beatrice_Tinsley
Galaxies with interacting gravitational fields
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Interacting_galaxy
American scientist
discoveries of high-z galaxies, and pioneering near-IR searches for protogalaxies (with various collaborators); discovery of the Fundamental plane (elliptical
Stanislav_George_Djorgovski
Comparison of a large range of energies
Wesley; Fryer, Chris L. (August 2013). "The Supernova That Destroyed a Protogalaxy: Prompt Chemical Enrichment and Supermassive Black Hole Growth". The
Orders_of_magnitude_(energy)
Astronomical objects
as mentioned before, conditions are favorable. This holds true for protogalaxies, or galaxies just thought to be forming, and old galaxies that have
List_of_ring_galaxies
American theoretical physicist (1904–1968)
Herman, Robert (1967). "Thermal Cosmic Radiation and the Formation of Protogalaxies". Proceedings of the National Academy of Sciences of the United States
George_Gamow
Radio galaxy located in the constellation Lynx
base of the jet. It is theorized B2 0902+34 might be a giant elliptical protogalaxy based on its spectrum, its luminosity of its continuum source, and the
B2_0902+34
Gas condensation following the Big Bang
galactic formation, with the supergalactic condensation fragmenting into protogalaxies. The formation of plane concentrations would compress the gas through
Zeldovich_pancake
Galaxy protocluster in the constellation Phoenix
how galaxy clusters develop is not complete. Farthest protoclusters Protogalaxy Zhou, Dazhi; Chapman, Scott C.; Aravena, Manuel; Araya-Araya, Pablo;
SPT2349-56
Aggregation of galaxies with 50 or fewer members
They are the smaller form of protoclusters. These contain galaxies and protogalaxies embedded in dark matter haloes that are in the process of fusing into
Galaxy_group
Citizen science project
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Radio_Galaxy_Zoo
Concept in astronomy
mechanical energy into the infalling gas was large enough to unbind the protogalaxy in one crossing time. The Silk and Rees model predicts a slope for the
M–sigma_relation
Galaxy filament
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Lynx–Ursa_Major_Filament
Proportional counter Propulsion Propulsive efficiency Prosper-René Blondlot Protogalaxy Proton Proton-to-electron mass ratio Proton Synchrotron Proton Synchrotron
Index_of_physics_articles_(P)
Galaxy with an annular appearance
as mentioned before, conditions are favorable. This holds true for protogalaxies, or galaxies just throughout to be forming, and old galaxies that have
Ring_galaxy
Galaxy filament
galaxy Halo corona Galactic plane Galactic ridge Interstellar medium Protogalaxy Galaxy filament Spiral arm Supermassive black hole Ultramassive Active
Ursa_Major_Filament
galaxy Faint blue galaxy Galaxy color–magnitude diagram Illustris project Protogalaxy Metallicity § Stars Cosmos Redshift 7 Large quasar group § List of LQGs
Outline_of_galaxies
English astrophysicist (born 1984)
Very Large Array to make the first detailed study of the evolution of protogalaxies in the early universe and came up with a creative alternative which
Jamie_Farnes
Lyman-break galaxy in the constellation Aquarius
could be interpreted either as the result of a merger of two smaller protogalaxies or as the fragmentation of dense gas clouds within a single dark matter
PAN-z14-1
Radio galaxy in the constellation Fornax
14 A. The galaxy has an extremely blue V - I color indicating it as a protogalaxy in the midst of forming the first stars in a low-dust medium. The second
MRC_0316−257
Radio galaxy in the constellation Cygnus
at 2 < Z < 4: Evidence That Some High-Redshift Radio Galaxies May Be Protogalaxies". The Astrophysical Journal. 411: 67. Bibcode:1993ApJ...411...67E. doi:10
4C_+48.48
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