What is the translation of " BINARY STAR " in Slovenian?

• binarna zvezda
• binarni zvezdni
• dvojna zvezda
• dvojnega zvezdnega

Examples of using Binary star in English and their translations into Slovenian

Binary Star is also a road novel.
Bonavia je torej tudi roman o poti.

He is credited with having discovered 1340 binary stars.
Odkril je 1340 dvojnih zvezd.

HD 1185 is a binary star[6] in the constellation Andromeda.
HD 1185 je binarna zvezda[1] v ozvezdju Andromede.

Oumuamua likely came to our solar system from a binary star system.
Oumuamua bi lahko prišel iz sistema dvojne zvezde.

Short orbital-period binary star detected at the heart of the planetary nebula M 3-1.
Kratka orbitalna binarna zvezda je zaznana v središču planetarne meglene M 3-1.

Along with Carl Vogel, Pickering discovered the first spectroscopic binary stars.
Pickering velja poleg Vogla za odkritelja prvih spektroskopskih dvojnih zvezd.

It's Albireo. It's a binary star system.
Imenuje se Albireo, to je binarni zvezdni sistem.

Many stars are gravitationally bound to other stars, forming binary stars.
Veliko zvezd je gravitacijsko vezanih z drugimi zvezdami in tvorijo dvojne zvezde.

KIC 9832227 is a contact binary star system in the constellation of Cygnus, located about 1800 light-years away.
KIC 9832227 je binarni zvezdni sistem, od Zemlje oddaljen približno 1.800 svetlobnih let.

Astronomers have discovered the first planet known to orbit a binary star system.
Astronomi so končno našli prvi Zemlji podoben planet, ki je del binarnega zvezdnega sistema.

Andromedae is a binary star[3] system in the northern constellation of Andromeda, near the northern border with Perseus.
Andromede je binarna zvezda v severnem ozvezdju Andromede, blizu severnega roba s Perzejem.

The most numerous sources of gravitational waves are binary stars systems.
Najprepričljivejši dokaz za obstoj gravitacijskih valov do danes predstavljajo sistemi binarnih zvezd.

All of these X-ray binary star systems are old, so they only reveal information about what happens much later, in their life.
Vsi ti rentgenski sistemi dvojnih zvezd so stari, zato nam razkrivajo le to, kaj se dogaja veliko pozneje v njihovem življenju.

As William Herschel discovered, many stars have close companions forming a binary star system.
Herschel je odkril, da imajo številne zvezde partnerja. Tvorijo binarni zvezdni sistem.

Zeta Oph was likely once a member of a binary star system, its companion star was more massive and hence shorter lived.
Zeta Oph je verjetno nekdaj bila del dvojnega zvezdnega sistema, kjer je bila njena spremljevalka masivnejša in je posledično tudi manj časa živela.

There was already evidence of gravitational waves from observations of binary star systems.
Doslej so obstajali zgolj posredni dokazi o obstoju gravitacijskih valov, denimo sistemi binarnih zvezd.

Γ Arietis, with a common name of Mesarthim, is a binary star with two white-hued components, located in a rich field of magnitude 8- 12 stars..
Γ Ovna, z pogostim imenom Mesartim, je binarna zvezda z dvema belima komponentama. Nahaja se v gostem polju 8.- 12. magnitudnih zvezd..

NASA's Chandra X-ray Observatory in orbit and an X-ray image of a binary star system black hole.
Nasin observatorij Chandra za preučevanje rentgenskih žarkov v orbiti in rentgenski posnetek dvojnega zvezdnega sistema črne luknje.

Modelling lightcurves of eclipse binary stars in crucial in order not to confuse them with planetary transits, that are the main targets of the Kepler mission.
Poznavanje in merjenje svetlobnih krivulj eklipsnih dvojnih zvezd je ključnega pomena, zato da jih ne zamenjujemo s prehodi planetov, ki so glavni cilj misije Kepler.

HD 224635 and HD 224636 is a pair of stars comprising a binary star system in the constellation Andromeda.
HD 224635 in HD 224636 je par zvezd, ki oblikujeta binarni zvezdni sistem v ozvezdju Andromede.

The red circles in this Chandra Observatory X-ray image identify a group of a dozen black holes that are members of binary star systems.
Rdeči krogi na tej rentgenski sliki Observatorija Chandra označujejo ducat črnih lukenj, ki so članice dvojnih zvezdnih sistemov.

After 1909, the instruments were also used to observe binary stars and perform photometry of nebulae.[3].
Po letu 1909 so se instrumenti uporabljali tudi za opazovanje dvojnih zvezd, izvajali so pa tudi fotometrijo meglic.[1].

Its brightest star, Alpha Andromedae, is a binary star that has also been counted as a part of Pegasus, while Gamma Andromedae is a colorful binary and a popular target for amateur astronomers.
Njena najsvetlejša zvezda, Alfa Andromede, je dvojna zvezda, ki se je nekdaj prištevala tudi k Perzeju. Gama Andromede je barvna dvojna zvezda in priljubljena tarča amaterskih astronomov.

Omega Andromedae(ω And, ω Andromedae) is the Bayer designation for a slowly co-rotating binary star system[9] in the northern constellation of Andromeda.
Omega Andromede(ω And, ω Andromede) je Bayerjevo poimenovanje za počasi se vrtečo binarno zvezdo v severnem ozvezdju Andromede.

This makes it possible on Earth to indirectly observe the gamma radiation generated by“wild” astronomical processes, such as objects falling into black holes in the centres of galaxies, supernova remnants and X-ray binary stars.
Na ta način lahko tudi na površju Zemlje posredno opazujejo sevanje gama, ki nastaja v“divjih” astronomskih procesih, kot so padanje snovi v črne luknje v središčih galaksij, ostanki supernov in rentgenske dvojne zvezde.

The ULXs are so called because they actually do radiate 10 to 1,000 times more x-ray power than"ordinary" x-ray binary stars, which harbor a neutron star or stellar mass black hole.
ULX se imenujejo zato, ker v resnici oddajajo 10 do 1000 krat več rentgenskega sevanja kot"navadne" rentgenske dvojne zvezde, ki nosijo nevtronsko zvezdo ali zvezdno črno luknjo.

However, K2 data complemented by follow-up spectroscopic observations with ground based observatories, including Keck telescope, Nordic Optical Telescope(NOT) and McDonald Observatory, indicate that EPIC 219654213 is a binary star.
Vendar pa podatki K2, dopolnjeni s spremljajočimi spektroskopskimi opazovanji z zemeljskimi opazovalci, vključno s teleskopom Keck, optičnim teleskopom Nordic Optical Telescope(NE) in Observatorijem McDonald, kažejo, da je EPIC 219654213 binarna zvezda.

This discovery provides the first direct evidence supporting the long-held belief that Type Ia supernovae come from binary star systems containing a normal star and a burned-out white dwarf star..
To odkritje je prvi neposredni dokaz, ki podpira trdno prepričanje, da supernove tipa Ia prihajajo iz binarnih zvezdnih sistemov, ki vsebujejo normalno zvezdo in izgorelo belo zvezdo.

The two stars were known to the Bedouin as"qarna al-hamal","horns of the ram".[30] It is 59 light-years from Earth.[31] It has a luminosity of 11 L☉ and its absolute magnitude is 2.1.[29] It is a spectroscopic binary star, one in which the companion star is only known through analysis of the spectra.[32] The spectral class of the primary is A5.[12] Hermann Carl Vogel determined that Sheratan was a spectroscopic binary in 1903; its orbit was determined by Hans Ludendorff in 1907.
Dve zvezdi sta bili Beduinom znani kot"qarna al-hamal","rogovi ovna".[30] Od nas je oddaljena 59 svetlobnih let.[31] Ima izsevnost 11 L☉ in absolutno magnitudo 2,1.[29] To je spektroskopska dvojna zvezda, saj je spremljevalka glavne zvezde znana le glede na analizo spektra.[32] Spektralni razred glavne zvezde je A5.[12] Hermann Carl Vogel je leta 1903 določil, da je to binarna zvezda; njeno tirnico je določil Hans Ludendorff leta 1907.

Located outside the triangle near Beta, Delta Trianguli Australis is the fourth-brightest star at apparent magnitude +3.8.[9] It is a yellow giant of spectral type G2Ib-II and lies 606 light-years(186 parsecs) away.[20] A binary star, it has a 12th-magnitude companion star separated by 30 arcseconds from the primary.[21] Lying halfway between Beta and Gamma, Epsilon Trianguli Australis is an optical double.
Nahaja zunaj trikotnika bližini Beta, Delta Trianguli Australis je četrti-najsposobnejših zvezda na navidezno magnitudo +3.8.[1] je rumeno velikan spektralnega tipa G2Ib-II in laži, 606 svetlobno leto(186 parsek) stran.[1] A binarni star, to je 12. -obseg spremljevalec star ločeni s 30 arcseconds iz primarne.[1], ki Leži na pol poti med Beta in Gama, Epsilon Trianguli Australis je optični dvojno.