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Class of astronomical objects
A symbiotic binary is a type of binary star system, often simply called a symbiotic star. They usually contain a white dwarf with a companion red giant
Symbiotic_binary
Binary star in the constellation Dorado
WOH G64 (IRAS 04553–6825) is a symbiotic binary in the Large Magellanic Cloud, roughly 50 kiloparsecs (163,000 light-years) from Earth. The primary component
WOH_G64
System of two stars orbiting each other
A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars are among
Binary_star
X-ray source that only emits soft X-rays
CAL 83 (LMC), CAL 87 LMC), and 1E 0035.4-7230 (SMC). A symbiotic binary star is a variable binary star system in which a red giant has expanded its outer
Supersoft_X-ray_source
Class of binary stars
X-ray emitting accretor. Low-mass X-ray binaries (LMXBs) Soft X-ray transients (SXTs) Symbiotic X-ray binaries Super soft X-ray sources or Super soft sources
X-ray_binary
Symbiotic binary
ZZ Canis Minoris is a symbiotic binary in the constellation Canis Minor. It is 4,000 light-years distant and is not visible to the naked eye with a maximum
ZZ_Canis_Minoris
Star whose brightness fluctuates, as seen from Earth
but larger superoutbursts. These binary systems usually have orbital periods of under 2.5 hours. These symbiotic binary systems are composed of a red giant
Variable_star
Planetary nebula in the constellation Norma
unusual PN in that it is believed, by some researchers, to contain a symbiotic binary at its center. One study suggests that the dense nebular gas at its
Mz_3
Collapsed core of a massive star
stars that have been detected are pulsars or a part of a binary system. Neutron stars in a binary system with a main sequence star can pull in large amounts
Neutron_star
Planet with helium-dominated atmosphere
transfer in a close binary system with a second, massive object like a neutron star. One scenario involves an AM CVn type of symbiotic binary star composed
Helium_planet
Triple star system in the constellation Scutum
hot component is itself a close binary, making the overall system a triple. It was once thought to be a symbiotic binary, exhibiting unique spectral emission
FR_Scuti
Constellation in the northern celestial hemisphere
2013. Mikołajewska, J.; Kenyon, S. J. (1992). "On the Nature of the Symbiotic Binary AX Persei". The Astronomical Journal. 103 (2): 579–92. Bibcode:1992AJ
Perseus_(constellation)
Binary star system in the constellation Andromeda
EG Andromedae (often abbreviated to EG And) is a symbiotic binary in the constellation Andromeda. Its apparent visual magnitude varies between 6.97 and
EG_Andromedae
Variable star in the constellation Andromeda
is a binary star system consisting of a red giant and a white dwarf. It is the prototype of a type of cataclysmic variable star known as symbiotic variable
Z_Andromedae
Constellation in the northern celestial hemisphere
Maciej; Polidan, Ronald S.; Slovak, Mark H. (1993). "Evolution of the symbiotic binary system AG Pegasi - The slowest classical nova eruption ever recorded"
Pegasus_(constellation)
Binary star in the constellation Monoceros
MWC 560 is a symbiotic binary star system in the equatorial constellation of Monoceros. The identifier comes from the Mount Wilson Calatogue of class O
MWC_560
Mansi M. (1 August 2022). "SRGA J181414.6-225604: A New Galactic Symbiotic X-Ray Binary Outburst Triggered by an Intense Mass-loss Episode of a Heavily
List_of_largest_stars
Cool giant star with approximately equal quantities of carbon and oxygen in its atmosphere
example of an extrinsic S star. It is a slow irregular variable in a symbiotic binary system with a hotter companion which may also be variable. The Mira
S-type_star
Supernova in the constellation Sagittarius
Suggested classical nova counterparts for 386 Designation Comments V1223 Sgr Intermediate polar V3890 Sgr Known recurrent nova Four further symbiotic binaries
SN_386
Variable star in the Cygnus constellation
Cygni (CH Cyg / HIP 95413 / BD +49 2999) is a red giant, variable, symbiotic binary in the constellation Cygnus. CH Cygni has a mass of 2 M☉ and a radius
CH_Cygni
Katynski, Marcus (2019-04-05). "FUSE Spectroscopic Analysis of the Slowest Symbiotic Nova AG Peg During Quiescence". The Astrophysical Journal. 874 (2): 178
List_of_smallest_known_stars
Substellar object
dwarfs binaries of type M, L, and T are less common with a lower mass of the primary. L-dwarfs have a binary fraction of about 24+6 −2% and the binary fraction
Brown_dwarf
Slow irregular eruptive variable stars
hdl:10722/179631. S2CID 121786223. Mikołajewska, J. (2007). "Symbiotic Stars: Continually Embarrassing Binaries". Baltic Astronomy. 16: 1–9. Bibcode:2007BaltA..16
Symbiotic_nova
Stellar core remnant
dwarf is Sirius B, at 8.6 light years, the smaller component of the Sirius binary star. In 1910, Henry Norris Russell, Edward Charles Pickering and Williamina
White_dwarf
Evolutionary theory
chloroplasts were originally independent organisms that merged into a symbiotic relationship with other one-celled organisms dates back to the 19th century
Symbiogenesis
Two pulsars orbiting each other
A binary pulsar is a pulsar with a binary companion, often a white dwarf or neutron star. (In at least one case, the double pulsar PSR J0737-3039, the
Binary_pulsar
Constellation in the southern celestial hemisphere
Drechsel, H.; et al. (2000). "A Photometric Study of the Eclipsing Symbiotic Binary AR Pavonis". Monthly Notices of the Royal Astronomical Society. 311
Pavo_(constellation)
American mathematician
an astronomer and mathematician who studies planetary nebulae and symbiotic binary stars. Lutz was the Boeing Distinguished Professor of Mathematics and
Julie_Lutz
Type of neutron star with beams of radiation
useful tools for astronomers. For example, observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence of gravitational
Pulsar
Globular cluster in the constellation Centaurus
These are the common or notable types of stars in the cluster. For the binary stars, the spectral class here is the primary stars’ spectral class. A 2008
Omega_Centauri
American astronomer and mathematician who studies planetary nebulae and symbiotic binary stars Sonja Lyttkens (1919–2014), Swedish mathematician, first Swedish
List_of_women_in_mathematics
Small number of stars that orbit each other
bodies (such as comets). A star system of two stars is known as a binary star, binary star system or physical double star. Systems with four or more components
Star_system
Variable star in the constellation Draco
Martino, Domitilla (December 2003). "X-ray observations of 4 Draconis: symbiotic binary or cataclysmic triple?". Monthly Notices of the Royal Astronomical
4_Draconis
Common gas atmosphere of a binary star system
envelope (CE) is gas that contains a binary-star system. The gas does not rotate at the same rate as the embedded binary system. A system with such a configuration
Common_envelope
Variable star in the constellation Vulpecula
ring-like structure. Infrared observations in 1980 suggested this is a symbiotic binary star system consisting of a variable, evolved star that has expanded
PU_Vulpeculae
Recurrent nova in the constellation Corona Borealis
T Coronae Borealis is a binary star and a recurrent nova about 3,000 light-years (920 parsecs) away in the constellation Corona Borealis. T Coronae Borealis
T_Coronae_Borealis
Coming together of two stars
by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms
Stellar_collision
Supernova that ejects a large mass at unusually high velocity
accelerates material away from the explosion at close to the speed of light. Binary systems are increasingly being studied as the best method for both stripping
Hypernova
Star in the constellation Microscopium
DD Microscopii is cataloged as a Z Andromedae variable, a type of symbiotic binary with occasional outbursts. It fluctuates between magnitudes 11.0 and
DD_Microscopii
Comparison of a large range of energies
Mena, Olga (28 December 2010). "High Energy Neutrinos from Novae in Symbiotic Binaries: The Case of V407 Cygni". Physical Review D. 82 (12) 123012. arXiv:1008
Orders_of_magnitude_(energy)
Star in the constellation Pegasus
AG Pegasi is a symbiotic binary star in the constellation Pegasus, composed of a red giant and white dwarf which are separated by 2.5 astronomical units
AG_Pegasi
Star in the constellation of Aquarius
constellation Aquarius. R Aquarii is a symbiotic star containing a red giant primary and a white dwarf secondary in a binary system. The orbital period is approximately
R_Aquarii
Large self-illuminated object in space
formed stars are in binary systems. In the model that best explained the data, all stars initially formed as binaries, though some binaries later split up
Star
Star in the constellation Lepus
A1 V, and a red giant with a class of M6III. The close pair form a symbiotic binary with ongoing mass transfer from the giant to the hotter component.
17_Leporis
Stellar classification
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
G-type_main-sequence_star
Double stars that show a significant interaction between their components
An Interacting binary star is a type of binary star in which one or both of the component stars has filled or exceeded its Roche lobe, also known as a
Interacting_binary_star
Scatter plot of stars showing the relationship of luminosity to stellar classification
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Hertzsprung–Russell_diagram
Dim, low mass stars on the main sequence
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Red_dwarf
Brief thermal runaway nuclear fusion in the core of low-mass stars
carbon–oxygen white dwarf. When hydrogen gas is accreted onto a white dwarf from a binary companion star, the hydrogen can fuse to form helium for a narrow range
Helium_flash
Type of large cool star
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Red_giant
Black hole formed by a collapsed star
a merger event of two smaller black holes. As of June 2020[update], the binary system 2MASS J05215658+4359220 was reported to host the smallest-mass black
Stellar_black_hole
Creation of chemical elements within stars
k_{r}} where kr is the reaction rate constant of each single elementary binary reaction composing the nuclear fusion process; k r = ⟨ σ ( v ) v ⟩ {\displaystyle
Stellar_nucleosynthesis
Type of emission nebula created by dying red giants
a wide variety of shapes and features are not yet well understood, but binary central stars, stellar winds and magnetic fields may play a role. The first
Planetary_nebula
Light from the stars
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Starlight
Structure formed by diffuse material in orbital motion around a massive central body
as compared to around 0.7 percent for nuclear fusion processes. In close binary systems the more massive primary component evolves faster and has already
Accretion_disk
Gravitational process studied in astronomy
the formation of a single star, must also account for the statistics of binary stars and the initial mass function. Most stars do not form in isolation
Star_formation
Type of star, larger and brighter than the Sun
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Giant_star
measured using a V-band filter in the UBV photometric system. Stars in binary systems (or other multiples) are listed by their total or combined brightness
List_of_brightest_stars
Italian-American astrophysicist
Trieste, Italy. Early in his career, Pesce conducted research into symbiotic binary stars and the atmospheres of late-type (AGB) giant stars at the Center
Joseph_E._Pesce
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Lists of stars by constellation
Lists_of_stars_by_constellation
Hypothetical compact star
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Q_star
Grouping of stars by similar metallicity
small ultra metal-poor star, slightly smaller than the Sun, found in a binary system of the spiral arms in the Milky Way. The discovery opens up the possibility
Stellar_population
Astronomer
Feast and Glass discovered the infrared/optical counterpart of the symbiotic binary x-ray source GX1+4. In 1978 Glass located the obscured x-ray source
Ian_Glass
Theoretical stellar remnant
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Black_dwarf
X-ray source
It was described as the birth of a symbiotic X-ray binary, a "first" in the lifecycle of an interacting binary star, or a zombie neutron star brought
IGR_J17329-2731
Classification in astronomy
neutrons, with a light scattering of protons and electrons. In certain binary stars containing a white dwarf, mass is transferred from the companion star
Compact_object
Astronomical category of stars
astronomy, the term iron star has been used for two observed types of star: Binary stars with highly variable emission and stellar spectral type Fe a blue
Iron_star
Binary star system in the constellation Cetus
Mira, pronounced /ˈmaɪrə/, is a binary star system in the constellation Cetus. It has the Bayer designation Omicron Ceti, which is Latinized from ο Ceti
Mira
Hypothetical early-universe star with a black hole core
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Quasi-star
American astrophysicist
astrophysicist. His work has included advances in symbiotic and other types of interacting binary stars, the formation and evolution of stars, and the
Scott_Jay_Kenyon
Changes to stars over their lifespans
transfer in a binary system may cause an initially stable white dwarf to surpass the Chandrasekhar limit. If a white dwarf forms a close binary system with
Stellar_evolution
Pattern of stars recognized on Earth's night sky
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Asterism_(astronomy)
Organism that lives within the body or cells of another organism
endosymbiosis) is a prime example of this modality. The Rhizobia-legume symbiotic relationship is important for processes such as the formation of root
Endosymbiont
Hypothetical hybrid star type
a binary system when one of the two stars goes supernova. Because no supernova is perfectly symmetric, and because the binding energy of the binary changes
Thorne–Żytkow_object
Study of the movement of stars
Way, which are interpreted as the result of gravitational encounters of binary stars with the supermassive black hole at the Galactic Center. Stellar kinematics
Stellar_kinematics
Type of neutron star with a strong magnetic field
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Magnetar
Isolated, small, and opaque nebula
Zinnecker, H. (10–15 April 2000). "Binary and multiple star formation in Bok globules". Birth and Evolution of Binary Stars, Poster Proceedings of IAU Symposium
Bok_globule
Hypothetical types of stars
observations interpreted as originating in a black hole binary could really originate in a boson star binary. The invisible companion to a Sun-like star identified
Exotic_star
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
AzV 65 AzV 76 AzV 78 AzV 367 Barbá 2-2 BP Crucis (Wray 977 or GX 301-2), binary with a pulsar companion. Cygnus OB2-12 HD 5291 (Sk 56) HD 32034 (R62 in
Hypergiant
Hypothesized alternative to a black hole
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Gravastar
Main sequence star that is more luminous and bluer than expected
found among field stars, as a result of close binary interaction. Since the fraction of close binaries increases with decreasing metallicity, blue stragglers
Blue_straggler
Type of stellar collision
observed GW170817, a gravitational wave associated with the merger of a binary neutron star (BNS) system in NGC 4993, an elliptical galaxy in the constellation
Neutron_star_merger
Type of star that is massive and luminous
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Supergiant
Class of young variable stars
dissipate on timescales of up to 10 million years. Most T Tauri stars are in binary star systems. In various stages of their life, they are called young stellar
T_Tauri_star
Changed position of star vs background
so the work is generally done only for sources like pulsars and X-ray binaries, where the radio emission is strong relative to the optical emission.[citation
Stellar_parallax
Outermost layer of a star's atmosphere
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Stellar_corona
Stars with irregular large fluctuations in brightness
brightness appeared as new stars in the sky. Cataclysmic variable stars are binary stars that consist of two components; a white-dwarf primary, and a mass-transferring
Cataclysmic_variable_star
Angular motion of a star about its axis
over 1000 times less effective at the end of the main sequence. A close binary star system occurs when two stars orbit each other with an average separation
Stellar_rotation
Gas and dust surrounding a newly formed star
stars differ from the disks surrounding the primary components of close binary systems with respect to their size and temperature. Protoplanetary disks
Protoplanetary_disk
Stars with a supergiant luminosity class with a spectral type of K or M
have acquired it after reaching the red supergiant stage, perhaps through binary interaction. The cores of red supergiants are still rotating and the differential
Red_supergiant
Star's outer shell from which light is radiated
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Photosphere
Central region of the Sun
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Solar_core
Light emitted by the Sun
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Sunlight
Stellar classification
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
K-type_main-sequence_star
Astrophysical phenomenon
hydrogen by binary interactions. Binary models provide a better match for the observed supernovae, with the proviso that no suitable binary helium stars
Supernova
Compact exotic star which forms matter consisting mostly of quarks
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Quark_star
Early stage in the process of star formation
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Protostar
Star not gravitationally bound to any galaxy
diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary system
Intergalactic_star
Hot, luminous star with a spectral type of A9 or earlier
type B5Ia UW Canis Majoris (UW CMa), two blue (O-type) supergiants in a binary system Zeta Puppis (Naos), a blue (O-type) supergiant, spectral type O4I(n)fp
Blue_supergiant
Species of sea anemone
radiation (PAR) to fuel the photosynthetic process. This restricts the symbiotic organism to euphotic habitats and requires consistent exposure to high
Aggregating_anemone
SYMBIOTIC BINARY
SYMBIOTIC BINARY
Girl/Female
Spanish
The laurel tree or sweet bay tree symbolic of honor and victory.
Boy/Male
Muslim
Symbolic
Girl/Female
American, Australian, British, English, Latin
Laurel Tree; Sweet Bay Tree Symbolic of Honor and Victory
Girl/Female
Hindu
Image, Beautiful, Symbol, Symbolic
Girl/Female
Hindu
Image, Beautiful, Symbol, Symbolic
Girl/Female
Tamil
Ojaswita | ஓஜஸà¯à®µà¯€à®¤à®¾
Bright brightness, A person symbolic of brightness
Ojaswita | ஓஜஸà¯à®µà¯€à®¤à®¾
Girl/Female
Hindu
Image, Symbolic
Girl/Female
Arabic, Muslim
Symbolic
Girl/Female
English
The laurel tree or sweet bay tree symbolic of honor and victory.
Girl/Female
Hindu, Indian
Brightness; A Person Symbolic of Brightness
Girl/Female
Hindu
Bright brightness, A person symbolic of brightness
Girl/Female
Tamil
Prathika | பà¯à®°à®¤à¯€à®•à®¾Â
Image, Beautiful, Symbol, Symbolic
Prathika | பà¯à®°à®¤à¯€à®•à®¾Â
Girl/Female
Hindu
Image, Beautiful, Symbol, Symbolic
Girl/Female
Tamil
Praatika | பà¯à®°à®¾à®¤à¯€à®•à®¾
Image, Symbolic
Praatika | பà¯à®°à®¾à®¤à¯€à®•à®¾
Girl/Female
Assamese, Bengali, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Tamil, Telugu
Symbol; Shadow; Lord Indra; Symbolic; Proud
Boy/Male
Indian
Symbolic
Girl/Female
Tamil
Pratika | பà¯à®°à®¤à®¿à®•à®¾
Image, Beautiful, Symbol, Symbolic
Pratika | பà¯à®°à®¤à®¿à®•à®¾
Girl/Female
Spanish
The laurel tree or sweet bay tree symbolic of honor and victory.
Girl/Female
Tamil
Prateeka | பà¯à®°à®¤à®¿à®•à®¾
Image, Beautiful, Symbol, Symbolic
Prateeka | பà¯à®°à®¤à®¿à®•à®¾
Girl/Female
Muslim
Symbolic
SYMBIOTIC BINARY
SYMBIOTIC BINARY
Boy/Male
Tamil
Sridatta | à®·à¯à®°à¯€à®¤à®¤à¯à®¤à®¾
Given by God
Girl/Female
Indian
Powerful, Strong
Girl/Female
Arabic
Singer
Girl/Female
Indian
Capable one
Boy/Male
Indian, Sanskrit
Quiver
Boy/Male
British, Christian, English, French, German
Heron Bird; Simple
Boy/Male
Tamil
Bee
Boy/Male
Bengali, Indian, Kannada, Tamil
Freedom; Self-determination
Boy/Male
Australian, British, English
Dream; Ash-tree Meadow
Surname or Lastname
English
English : topographic name for someone who lived in a short, straight valley, from Middle English combe (see Coombe), + the suffix -er denoting an inhabitant.Americanized spelling of German Kummer.
SYMBIOTIC BINARY
SYMBIOTIC BINARY
SYMBIOTIC BINARY
SYMBIOTIC BINARY
SYMBIOTIC BINARY
a.
See Symbolics.
n.
Specifically :(a) The principles and practices of those in the Church of England, who in the development of the Oxford movement, so-called, have insisted upon a return to the use in church services of the symbolic ornaments (altar cloths, encharistic vestments, candles, etc.) that were sanctioned in the second year of Edward VI., and never, as they maintain, forbidden by competennt authority, although generally disused. Schaff-Herzog Encyc. (b) Also, the principles and practices of those in the Protestant Episcopal Church who sympathize with this party in the Church of England.
n.
A rude picture, as of a bird, beast, or the like, used by the North American Indians as a symbolic designation, as of a family or a clan.
n.
A binary compound of sulphur, or one so regarded; -- formerly called sulphuret.
a.
Bringing a conception or notion directly before the mind; presenting an object to the memory of imagination; -- distinguished from symbolic.
a.
Alt. of Symbolical
n.
A hypothetical radical, SO4, regarded as forming the acid or negative constituent of sulphuric acid and the sulphates in electrolytic decomposition; -- so called in accordance with the binary theory of salts.
a.
Of or pertaining to the signs or symptoms of diseases.
n.
A binary compound of sulphion, or one so regarded; thus, sulphuric acid, H/SO/, is a sulphionide.
a.
Alt. of Semiotic
v. t.
To make representative of something; to regard or treat as symbolic.
n.
A binary compound of selenium, or a compound regarded as binary; as, ethyl selenide.
a.
Pertaining to, containing, or consisting in, an emblem; symbolic; typically representative; representing as an emblem; as, emblematic language or ornaments; a crown is emblematic of royalty; white is emblematic of purity.
n.
A basis for a numeral system; as, the decimal scale; the binary scale, etc.
a.
Relating to signs or indications; pertaining to the language of signs, or to language generally as indicating thought.
n.
A symbolic expression (by means of letters, figures, etc.) of the constituents or constitution of a compound.
n.
that branch of historic theology which treats of creeds and confessions of faith; symbolism; -- called also symbolic.
a.
Of or pertaining to a symbol or symbols; of the nature of a symbol; exhibiting or expressing by resemblance or signs; representative; as, the figure of an eye is symbolic of sight and knowledge.
n.
A binary compound of zinc.
a.
Same as Semeiotic.