COREPHYSICS

• Galastellides are semistable monocores of collapsed nucleons and nuclides.
• Galastellides are gravitypull attuned to other galastellides.
• Galastellides are teelstream attuned to any teelstream they are in.

• Galastellides are a nucleus, eventhorizon, teelosphere, gravitysheath, and gravitysheath interface.
• Galastellide nucleuses are a teelcore.
• Galastellide nucleuses may or may not contain solidbonded photides and morphides.
• Galastellide nucleuses may or may not contain liquidbonded photides and morphides.
• Galastellides may or may not have an atmosphere of gasbonded photides and morphides.
• Galastellides may or may not retain a stellasphere.
  

• Galastellides are stellides that peakmassed as galastars during semistabilisation.
• Galastellides reactivate as galastars if made sufficiently understable by further accretion.

• Galastars are understable galastellides.
• Galastars are primarily accretions of nucleons and nuclides.
• Galastars are blackstars with additional accretion.
• Galastars peakmass at 45 or more solarmasses.
• Galastar peakmasses are limited by the availability of accretables.
• Galastar semistabilisation is by gravitycollapse, emissioncollapse, fusioncollapse, ferriccollapse, fissioncollapse and stellaspherecollapse.
• Galastars are a nucleus, eventhorizon, bulge, stellasphere, teelosphere, and gravitysheath.

• Galastar nucleuses are a teelcore inside a teelocean.
• Galastar teelcores are a sphere/spheroid of solidbonded teels.
• Galastar teeloceans are a stratum of liquidbonded teels.
  
• Galastar teelcores spin.
• Galastar teelcores have a northpole, equator and southpole.
• Galastar teeloceans are teelstream systems.
• Galastar teelstream systems are driven by the teelcore spin.
• Galastar teelstream systems are centrifugal.
  
• Galastar nucleuses absorb teels from the teelosphere.
• Galastar nucleuses eject more teels into the teelosphere than they absorb.
  
• Teel absorption differentially adds gravityvelocity and massvelocity.
• Teel absorption increases nucleus understability.
• Nucleus semistabilisation is per gravitymass differential mechanism.

• Galastar teelospheres surround a galastar's nucleus.
• Galastar teelosphere are a stratum of gasbonded teels.
• Galastar teelospheres can extend beyond the stellasphere.
• Galastar teelospheres are teelstream systems.
• Galastar teelstream systems are driven by nucleus spin.
• Galastar teelstream systems can be axial, centrifugal, or chaotic as conditions dictate.
• Galastar teelstream systems can be a mix of axial, centrifugal, and chaotic as conditions dictate.
• Galastar teelospheres are understable.
• Galastars eject teels from the galastar as gravitycollapse.
  

• Galastar eventhorizons are the surface of the region surrounding a galastar nucleus within which escapevelocity exceeds lightspeed.
• Photons and heavier objects cannot escape across an eventhorizon.
• Fundamides and some neutrinos can escape across an eventhorizon.
• Teelstream systems cross the eventhorizon

• Galastar bulges are a region of engorged stars.
• Galastar bulges are outside the nucleus.
• Galastar bulges are outside the eventhorizon.
• Galastar bulges are inside the stellasphere.
• Bulge stars are absorbed from the stellasphere.
  
• Bulge stars are strongforced to the galastar nucleus.
• Bulge stars are strongforced to adjacent bulge stars.
• Bulge stars cannot approach the nucleus closely.
• Bulge stars "ride" on the dense inner teelosphere.
• Outer bulge stars are engorged by galastar teelstream system.
• Engorged stars contain overengorged nuclides.
• Overengorged nuclides dissipate.
• Engorged stars progressively become metalpoor.
• Outer bulge stars are progressively drawn toward the inner bulge.
  
• Inner bulge stars are overengorged by galastar teelstream system.
• Overengorged bulge stars contain overengorged morphides.
• Overengorged morphides progressively dissipate.
• Overengorged bulge stars dissipate into the teelosphere.

• Galastar stellaspheres are the stars and lesser objects that envelope the galastar bulge.
• Stellasphere objects are gasbonded to a galastar nucleus.
• Stellaspheres are "elliptical" or "spiral" as conditions dictate.
• Stellaspheres may be axial, centrifugal, or chaotic as conditions dictate.
• Galastar stellaspheres are understable.
• Stellaspheres absorb objects from beyond the galastar gravitysheath interface courtesy the nucleus gravitypull.
• Stellaspheres absorb lesser galastars as globulars.
• Globulars are progressively stripped of their stellasphere.
• Globular stars are made metalpoor by the galastar teelstreams.
• Galastars can merge / collide with other galastars of similar gravitymass.
• Galastars can be absorbed by larger galastars.
• Galastar stellaspheres are understable.
• Absorption increases stellasphere understability.
• Galastar stars semistabilise by gravitycollapse, emissioncollapse, fusioncollapse, ferriccollapse, and fissioncollapse as conditions dictate.
  
• Galastar stellaspheres semistabilise by emissioncollapse and gravitycollapse

• Globulars are stripped of their own stellaspheres by galastars teelstream systems.
• Globular stars are engorged by galastar teelstream system.
• Globular stars become progressively metalpoor.
• Most stellasphere stars are metalrich.
• Stellasphere stars are drawn to the bulge over time.
  
• Stellasphere stars lose metalrichness as they approach the bulge.

• Bulge stars are engorged or overengorged.
• Sufficient engorgement breaks nuclides into heliums.
• Sufficient overengorgement breaks heliums to neutrons and star dissipation.
• Sufficient overengorgement breaks neutrons to photides and fundamides.
• Photides and fundamides can be absorbed across the eventhorizon.

• NARRATIVE
• DESCRIPTION
• LIFECYCLE

• CAVEATS

• "SUPERONECOREGALAXIES"
• SINGULARITIES
• METALLICITY AND AGE IN STARS

• Current Paradigm:     classified by observable characteristics.
• Core Physics:     classified by the number of galaxycores in the nucleus.

• Rule of thumb:    Core Physics onecoregalaxies equate to higher mass dwarf galaxies and lower mass spiral galaxies.

• Nucleus     A galaxycore, inside a blackhole, inside an aurasphere.

• Galaxycore

• A galaxycore in a onecoregalaxy is a single teelcore.
• The teelcore is a sphere/spheroid of solidbonded pairs of adjacent teels.
• A galaxycore is spinning and thus has a northpole, equator, and southpole.
• A galaxycore's mass is enough to generate a blackhole.
• A galaxycore absorbs teels from the aurasphere.
  
• Energy and mass is differentially increased by additional teels.
• A galaxycore is engorged by a differential increase in energy and mass.
• Due to engorgement, energyvelocity exceeds massvelocity.
• Due to energyvelocity exceeding massvelocity, a galaxycore is understable.
• Due to understability, a galaxycore is stabilising per the energy/mass differential mechanism.
• A galaxycore stabilises by ejecting teels into the aurasphere.
• A midlife galaxycore is always understable to a greater or lesser degree.
  

• Blackhole

• A blackhole is a region inside which the escapevelocity is higher than lightspeed.
• The surface of a blackhole is its eventhorizon.
• The eventhorizon is outside the galaxycore.
• The eventhorizon is inside the the aurasphere.
• Photons and superphotonics cannot escape from a blackhole.
• There are no photons or superphotonics inside a blackhole.
  
• Subphotonics can escape from a blackhole if they exceed lightspeed.
• There are subphotonics inside a blackhole.
  
• The volume of a blackhole increases with galaxycore mass increases.
• The volume of a blackhole decreases with galaxycore mass decreases.

• Aurasphere

• An aurasphere is a stratum of liquidbonded teels surrounding the galaxycore.
• An aurasphere is a liquidbonded teelstream system.
• The teelstream system responds to the spin of the galaxycore.
  
• The teelstream system is centrifugal.
  
• An aurasphere absorbs teels ejected by the galaxycore.
• An aurasphere absorbs objects incoming from the bulge.
• Subphotonics and photons emitted by bulge stars.
• Stripped neutrons, deuteriums, and heliums gravitypulled from the bulge.
• An aurasphere dissipates objects absorbed from the bulge to teels.
• Energy and mass is differentially increased by additional teels.
• An aurasphere is engorged by a differential increase in energy and mass.
• Due to engorgement, energyvelocity exceeds massvelocity.
• Due to energyvelocity exceeding massvelocity, an aurasphere is understable.
• Due to understability, an aurasphere is stabilising per the energy/mass differential mechanism.
• An aurasphere stabilises by ejecting teels into the galaxycore and into the bulge.

• Bulge     A region of overengorged stars.

• A bulge is a region of overengorged stars inside a gasbonded  teelstream system.
• The teelstream system extends into (and often beyond) halosphere.
• The teelstream system responds to the movement of the aurasphere.
• The teelstream system is centrifugal overall.
• A bulge absorbs teels ejected by the aurasphere.
• A bulge absorbs subphotonics, photons, and superphotonics incoming from the halosphere:
• Teelstream system energy and mass is differentially increased by the absorptions.
• The differential increase in energy and mass understabilises the teelstream system.
• The understability of the teelstream system overengorges the bulge's stars.
  
• A bulge's stars are also overengorged by emission pressure.
• Overengorgement inhibits fusion in stars.
• Overengorgement breaks star isotopes to heliums, deuteriums, and neutrons.
• Overengorgement renders stars metalpoor.
• Overengorgement, over time, dissipates stars.
  
• A bulge's stars are stratified:
• Stratum 1:     Strongforced stars subforced to the aurasphere surface by galaxy intrinsic gravitypull.
• Stratum 2:     Strongforced but not subforced stars bound to the surface of Stratum 1 by galaxy intrinsic gravitypull.
• Stratum 3:     Not strongforced but still overengorged stars bound to the surface of Stratum 2 by galaxy intrinsic gravitypull.
• A bulge's packing density decreases from aurasphere surface outward.
• Star numbers increase as stars are absorbed from the halosphere.
• Star numbers decrease as stars are dissipated.
• A bulge stabilises by emitting photons, and ejecting subphotonics, into the halosphere.
• Bulge stabilisation is per the energy/mass differential mechanism.
  
• A onecoregalaxy bulge ejects most subphotonics equatorially.
  

• Halosphere     A region of gasbonded objects.

• A halosphere responds to the movement of the bulge.
• A halosphere is stars inside a gasbonded teelstream system.
• A halosphere teelstream system extends from the aurasphere surface to the surface of the halosphere - and often beyond.
  
• The teelstream system is centrifugal overall.
• A halosphere absorbs subphotonics and photons from the bulge.
• A halosphere absorbs subphotonics, photons, and superphotonics from the gravitysheath and beyond.
• Teelstream system energy and mass is differentially increased by the absorptions.
• The differential increase in energy and mass understabilises the teelstream system.
• A proportion of the absorptions are accreted by halosphere stars.
• Absorptions not accreted by stars are most of a halosphere's mass.
• A halosphere's stars are mostly in an equatorial disc.
• Low mass onecore galaxies have no equatorial disc.
• High mass onecore galaxies have arms of stars in the equatorial disc.
• Halosphere teelstream systems do not inhibit stellar fusion.
  
• A halosphere's volume increases with nucleus volume.
  
• Halospheres of sufficient volume, allied to nuclei of sufficient mass, can form star clusters bound by their own intrinsic gravitypull and in dominance adjacency.
• Halospheres of sufficient volume, allied to nuclei of sufficient mass, can accrete smaller galaxies and star clusters.
• Halosphere teelstream systems strip the halosphere from star clusters and accreted galaxies.
• Stripped star clusters and galaxies are globular clusters.
• A halosphere is understable if the bulge is understable.
• Halosphere stabilisation is by photon emission into the bulge.
• Halosphere stabilisation is by subphotonics and superphotonics being gravitypulled into the bulge.
  
• Halosphere stabilisation is by photon emission across the gravitysheath interface.
• Halosphere stabilisation is by equatorial ejection of subphotonics and superphotonics.
• Halosphere stabilisation is per the energy/mass differential mechanism.
  

• Gravitysheath     A region within which a onecoregalaxy's gravitypull is stronger than that of any other object.

• Onecoregalaxies begin as protogalaxies.
• A protogalaxy is a star cluster bound by intrinsic gravitypull.
• Protogalaxies have a gravitycentre.
• Protogalaxies are within a gravitysheath.
• Protogalaxies retain objects at the gravitycentre by trojan adjacency.
• The retained objects are anything from teels to stars.
• A protogalaxy's retained objects are its protonucleus.
• Protonuclei have masscentres.
• Protonuclei have extrinsic gravitypull
• Protonuclei have gravitysheaths inside the gravitysheaths of their protogalaxies.
• A protonucleus accretes from the protogalaxy and from beyond the protogalaxy.
• Protonuclei accretion commensurately increases protonuclei masses and extrinsic gravitypulls.
• Increasing extrinsic gravitypull commensurately increases the volume of protonuclei gravitysheaths.
• Increasing the volume of protonuclei gravitysheaths increasingly encloses protogalaxy stars.
• Enclosed stars are dominance adjacent to their protonuclei and type adjacent to adjacent stars.
• A protogalaxy becomes a onecoregalaxy when its protonucleus becomes a nucleus.
• A onecoregalaxy nucleus is:
• a single solidbonded galaxycore:
• inside a blackhole:
• inside a liquidbonded aurasphere.
• A onecoregalaxy is:
• a nucleus:
  
• inside a bulge:
• inside a halosphere:
• inside a gravitysheath.
• A low mass onecoregalaxy is a dwarf galaxy.
• Dwarf galaxies are bulges with little or no obvious halosphere.
• Dwarf galaxies are the most abundant type of galaxy.
• Dwarf galaxies are difficult to detect due to low luminosity, low mass, and small size.
• Hypothesis:     Dwarf galaxies form from the subphotonic ejections of understable galaxies that gather between galaxies in trojan adjacency.
• Dwarf galaxies without blackholes are not onecoregalaxies.
• Dwarf galaxies with blackholes are onecoregalaxies.
• Dwarf galaxies without blackholes can evolve into onecoregalaxies by accretion.
  
• A high mass onecoregalaxy is an unbarred spiral galaxy.
• Spiral galaxies are bulges surrounded by halospheres.
• The halosphere stars are mostly concentrated in a disc.
• Spiral galaxies are barred or unbarred.
• Barred spiral galaxy discs are polar.
• Barred spiral galaxies are twocoregalaxies.
  
• Unbarred spiral  galaxy discs are equatorial.
• Unbarred spiral galaxies are all onecoregalaxies.
• Hypothesis:     Unbarred spiral galaxies are dwarf galaxies that have grown by accretion.
• Barred spiral galaxies are roughly two thirds of known spiral galaxies.
• Unbarred spiral galaxies are roughly one third of known spiral galaxies.
• A midlife onecoregalaxy is understable.
• Stabilisation is by the emission of photons.
• Stabilisation is by the ejection of subphotonics and superphotonics.
• Stabilisation is per the energy/mass differential mechanism.
  
• An understable onecoregalaxy is simultaneously subject to accretion expansion and stabilisation contraction.
• If accretion expansion dominates stabilisation contraction, onecoregalaxies can grow.
• If stabilisation contraction dominates accretion expansion, onecoregalaxy can stabilise.
• During an understable onecoregalaxy's stabilisation:
• The halosphere content is drawn into the bulge.
• The bulge content is overengorged, broken, and drawn into the aurasphere.
• The aurasphere content is dissipated to teels and absorbed by the galaxycore.
• The understable galaxycore ejects excess teels into the aurasphere.
• The understable aurasphere ejects excess subphotonics into the bulge/halosphere teelstream system.
• The understable bulge/halosphere teelstream system ejects excess subphotonics across the gravitysheath interface.
• The stabilisation endpoint is either:
• the onecoregalaxy is a cold galaxy.
• the onecoregalaxy is in engorgement stasis.
  
• In practice, the endpoint for most onecoregalaxies is:
• to be absorbed by a larger galaxy.
• to strongforce to another onecoregalaxy to become a twocoregalaxy.
• to strongforce to a twocoregalaxy to become a threecoregalaxy.

• IC 1101:     "is a supergiant elliptical galaxy at the centre of Abell 2029 galaxy cluster and is one of the largest known galaxies. Its halo extends about 600 kiloparsecs from its core and it has a total of about 100 trillion stars. The galaxy is located 320 megaparsecs from Earth." (Wikipedia 15 Aug 2021)

• Current Paradigm

• Blackhole:   "A gravitationally domineering celestial body with an event horizon from which even light cannot escape; the most dense material in the universe, condensed into a singularity" (Wiktionary 22.07.2021).

• Singularity:   "A point or region in spacetime in which gravitational forces cause matter to have an infinite density, associated with black holes" (Wiktionary 22.07.2021).

• Core Physics

• The notion of a gravitational singularity is a logictrap.
• Logictrap:  conclusions drawn or assumptions made when information is missing or misinterpreted.
  
• In the Current Paradigm, repellence is not a fundamental property.
• In the Current Paradigm, subphotonics are not formally recognised.
• Teels have dimensions other than zero and are 100% repellent.
• Thus teels cannot be infinitely condensed.
  
• Thus there can be no singularity.

• Current Paradigm:

• "Population II, or metal-poor, stars are those with relatively little of the elements heavier than helium. These objects were formed during an earlier time of the universe." (Wikipedia 22.07.2021)
• 
  

• Core Physics:

• The belief that metalpoor stars are old stars is widespread.
• Metalpoor stars can be old but it is not being metalpoor that makes them so.
  
• Most bulge stars are metalpoor.
• Bulge stars are overengorged.
• The overengorgement breaks the star's isotopes to nucleons.
• Thus bulge stars are, or are becoming, metalpoor.
• Bulge stars dissipate into the aurasphere.
  
• Many halosphere stars are metalrich.
• Over time, halosphere stars are drawn into the bulge.
• Stars entering the bulge become overengorged.
• The overengorgement turns metalrich stars into metalpoor stars.
• That a star is metalrich or metalpoor is a consequence of the conditions it has endured. Not its age.