「super nova」の共起表現一覧(1語右で並び替え)
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| SN 1901B was a | supernova about 52.5 Mlys away in Messier 100, a spira |
| SN 1979C was a | supernova about 50 million light-years away in Messier |
| There appears to be no | supernova activity in these galaxies. |
| “When I'm dead (you should dance”)] from the | Supernova album considered to be the band's most famou |
| d observation, variable star photometry, and | supernova and nova discovery, and colorimetry and Pola |
| hat only a short time had passed between the | supernova and the time the meteorites had solidified a |
| Japanese releases of the game (Dancing Stage | SuperNova and Dance Dance Revolution SuperNova respect |
| r Dogs, and the games Dance Dance Revolution | SuperNOVA and Pop'n Music Carnival (13). |
| rse, as well as improved measurements of the | supernova, and X-ray properties of galaxy clusters. |
| These two events ( | supernova and solidification of gas cloud) were inferr |
| rossovers featured on Dance Dance Revolution | SuperNOVA, and later as part of a set of Bemani crosso |
| a pulsar is closer (and also resulted from a | supernova), and in 1998 another supernova remnant was |
| an encounter between the blast wave from the | supernova and a small isolated cloud. |
| The options menu was redesigned on | Supernova, and is still accessed by holding down the s |
| s of a lunar eclipse in 1569 and of the 1572 | supernova appearing in Cassiopeia, which he recorded o |
| Although | supernova are common, with one exploding every few sec |
| evidence (namely the observation of distant | supernova as standard candles, and the well-resolved m |
| t time that astronomers have ever observed a | supernova as it occurred. |
| S Andromedae, what they considered a typical | supernova, as an explosive event that released radiati |
| earless Records saw At the Drive-In open for | Supernova at a bar named Club Mesa. |
| chool was re-named Nova Hreod College; Nova ( | supernova) being the name a dying red star re-born int |
| pace, such as this galaxy (NGC 4526) and the | supernova beside it (SN 1994D). |
| e massive star that was destroyed in its own | supernova blast. |
| Supernova burst SN 2003cg has been observed in 2003. | |
| It is predicted that the star will | supernova, but there is still the possibility of Beta |
| ronomers theorized that it could have been a | supernova, but the unique filtering properties of the |
| prise intentionally causes 109 Piscium to go | supernova by entering warp drive too close to the star |
| Champagne | Supernova by Oasis |
| bjects such as minor planets and comets) and | supernova candidates are released in real time. |
| The spectral characteristics of the | supernova changed over time. |
| For season two, the band Rock Star | Supernova chose Lukas Rossi as the lead singer of thei |
| The | supernova, classified as a Type I supernova, reached a |
| V. has a joint venture in the USA, producing | SUPERNOVA cleaning compounds: NOVACHEM of Bridgeport, |
| ectroweak star is theorized to occur after a | supernova collapse. |
| gists to consider an extraterrestrial cause ( | supernova, comet, asteroid) for the extinction of the |
| The band | Supernova consisted of Gilby Clarke, Jason Newsted, an |
| e eventually extinguished on Neptune after a | supernova consumes the remains of the solar system. |
| osmology along with the other members of the | Supernova Cosmology Project for this work. |
| In 1998 this team, along with the | Supernova Cosmology Project, found evidence of the acc |
| ker and Saul Perlmutter, who had founded the | Supernova Cosmology Project in 1988 at Lawrence Berkel |
| awrence Berkeley National Laboratory and the | Supernova Cosmology Project (the set defined by the co |
| Such an aberrant type Ia | supernova could throw distances and other scientific w |
| SN 1998bw was a rare type I/Ib gamma ray | supernova detected on 26 April 1998 in the ESO 184-G82 |
| last of these is famous for being the first | supernova detected by the X-Rays released very early o |
| SN 2008D is a | supernova detected with NASA's Swift X-ray telescope. |
| SN 2005df was the 104th | supernova discovered in 2005. |
| SN 2007bi was an extremely energetic | supernova discovered early in 2007 by the internationa |
| SN 2005B, the second | supernova discovered in 2005, was discovered by amateu |
| It was a type Ia | supernova, Discovered by Zhangwei Jin and Xing Gao (Ch |
| SN 2001ig was a rare Type IIb | supernova discovered by Australian amateur Robert Evan |
| al number had already increased to 40 visual | supernova discoveries plus one comet. |
| with Robert Owen Evans, who had made several | supernova discoveries using Thompson's charts. |
| Supernova disruption of galactic disk gas; | |
| At live shows, | Supernova dress in silver jumpsuits and custom-made sp |
| tion since June 1992, and is a member of the | Supernova Early Warning System. |
| lei to the interstellar medium, or that each | supernova ejects only a very small amount of r-process |
| Such a | supernova event may pose some threat to life on the Ea |
| 999, King, Modjaz, & Li discovered the first | supernova ever detected in IC 1613. |
| Tin foil remains a major part of the | Supernova experience: fans are encouraged to wear foil |
| In the same way that | supernova experiments provide a "standard candle" for |
| it must be due to an asymmetry in the way a | supernova explodes. |
| It is believed to have been created by a | supernova explosion of its companion star about one mi |
| h fell due to some perturbation, perhaps the | supernova explosion responsible for Sgr A East. |
| 50 to 100 times more energy than a standard | supernova explosion to create a structure of this size |
| ollapse directly into a black hole without a | supernova explosion, which would eject most of its mas |
| duced too little radioactive 56Ni to power a | supernova explosion. |
| ich is thought to arise from a fairly recent | supernova explosion; only four are known to exist for |
| that this has been brought about by recorded | supernova explosions in the region, blowing away or de |
| into red supergiants and end their lives in | Supernova explosions within a few million years. |
| th a direct comparison between the impact of | supernova explosions and stellar winds on surrounding |
| Nuclear reactions in stars and | supernova explosions produce very large numbers of neu |
| Supernova explosions produce such heavy elements, so h | |
| n of massive stars, which sets the stage for | supernova explosions, helps explain how elements like |
| The Nearby | Supernova Factory project, based at Lawrence Berkeley |
| It has been referred to as the ' | Supernova Factory' as three supernovas have occurred t |
| for the understanding of dwarf galaxies and | supernova feedback (1986, 2003), for the analysis of l |
| Michael Rebello, 02, lead singer | Supernova Fieldtrip |
| Supernova Genesis | |
| stronomy article, a cheela realizes that the | supernova half a million human years ago created both |
| ut 15 million light-years away from us, this | supernova happened 15 million years ago. |
| The | supernova has been described as an unambiguous fit for |
| The | supernova has been linked to GRB 980425, which was det |
| Supernova has disbanded entirely, while INXS exists wi | |
| Apparently, the triple | supernova has opened a rift in space and time. |
| Hence, the | supernova has been classified as a type IIb, a interme |
| s, star clusters, nearby galaxies, GRBs, and | supernova have been observed from ARIES. |
| cks from their highly acclaimed debut album, | Supernova, have been included on 20 separate compilati |
| ery small, it appears very similar to a tiny | supernova, hence the term 'bosenova' - the nomenclatur |
| alia where he writes books and continues his | supernova hunting using a 12 inch (31 cm) reflecting t |
| With the | supernova imminent, the elated Elbrun informs Data he |
| a time”) in 1993, Rosa (“Pink”) in 1994 and | Supernova in 1997. |
| teur astronomer (Paulo Cacella) detected one | supernova in the southeastern part in March 2002 (SN 2 |
| SN 2011by was a | supernova in NGC3972. |
| SN 1999EC is a | supernova in Canis Major. |
| his solo tours.He also toured with Rockstar | Supernova in 2007 with Johnny Colt, Lucas Rossi, Gilby |
| The team was able to catch the | supernova in action because they had been making obser |
| SN 2005df was a Type Ia | supernova in galaxy NGC 1559. |
| At any rate, no | supernova in the Milky Way has been visible to the nak |
| father, and a friend spotted a magnitude 17 | supernova in galaxy UGC 3378 in the constellation Came |
| eaning that it will most likely explode as a | supernova in less than 20 million years. |
| other heavy elements into space during this | supernova including more than 6 solar masses of radioa |
| ost likely candidate for the remains of this | supernova is Geminga ("Gemini gamma-ray source"), a pu |
| A bosenova or bose | supernova is a very small, supernova-like explosion, w |
| Supernova is the second album of Polish band Exodus. | |
| hed details of his observations in 1574; the | supernova is now known as Tycho's Supernova. |
| 2012: | Supernova is a 2009 direct-to-video science fiction di |
| The | supernova is known as SN 2010cr and is located at 13:2 |
| Supernova is an American pop punk band formed in Costa | |
| Acleris | supernova is a species of moth belonging to the family |
| This type of | supernova is known as a core collapse and is the resul |
| released just the year before, Dancing Stage | SuperNova, it only took on the persona of the game wit |
| ated SNLS-03D3bb by the Canada-France-Hawaii | Supernova Legacy Survey and sometimes called the "Cham |
| SN 1998aq is a | supernova located in galaxy NGC 3982. |
| SN 2009gj was a | supernova located approximately 60 million light years |
| Such productions include Changi, | Supernova, Make or Break and False Witness. |
| rom Canada was reported to have discovered a | supernova, making her the youngest ever to find a supe |
| The remnant of this | supernova may be the nearest besides the Local Bubble, |
| pulsar kicks would give us insight into the | supernova mechanism. |
| The HALO (Helium and Lead Observatory) | supernova neutrino detector. |
| As expected for the remnant of a Type Ia | supernova, no associated neutron star or black hole ha |
| November - A | supernova, now designated as SN 1572 appears in the co |
| region of high neutron flux, such as during | supernova nucleosynthesis after core-collapse, and yie |
| urring in core-collapse supernovae (see also | supernova nucleosynthesis) responsible for the creatio |
| The only | supernova observed within this galaxy is SN 1969Q. |
| SN 1993J is a | supernova observed in the galaxy M81. |
| SN 1956A was the only | supernova observed in M109 since its discovery. |
| It was the only | supernova observed in the NGC 7752 and NGC 7753 galaxi |
| At the time, it was the second brightest | supernova observed in the twentieth century behind SN |
| The | supernova occurred in a galaxy some 4 billion light-ye |
| this composit image only one year after the | supernova occurred, and it had faded away at that time |
| A | supernova occurs when the core of a star collapses und |
| It was the 3rd brightest | supernova of 2008. |
| upplied the most detailed description of the | supernova of 1054. |
| lamsteed may have inadvertently observed the | supernova on August 16, 1680, when he catalogued a sta |
| ana Robichaux (the runner-up from Rock Star: | Supernova) on Ellen DeGeneres. |
| vations by Astron were those of the SN 1987A | supernova on March 4-12, 1987 and of Halley's Comet in |
| ctory automated wide-field survey detected a | Supernova on the outskirts of NGC 5177. |
| Spectrum of SN1998aq, a Type Ia | supernova, one day after maximum light in the B band |
| Dancing Stage | SuperNova, or DS SuperNova was released by Konami's Eu |
| al being fed into the object either from the | supernova or a binary companion. |
| r changes triggered by the collapse (such as | supernova or pulsations leading to a planetary nebula) |
| the heaviest elements which do not require a | supernova or similarly cataclysmic event for formation |
| h it is unknown whether it will explode in a | supernova or die off as a rare neon-oxygen white dwarf |
| lusters of galaxies, consistent with type II | supernova origin |
| a neutron star, previously introduced in the | supernova paper, is explained along with the idea of c |
| sted Michael Schwartz's telescope, active in | supernova patrols, until Tenagra Observatories opened |
| was featured on the reality show Rock Star: | Supernova, performed by Ryan Star. |
| The explosion of the | supernova precursor star, in the spiral galaxy NGC 277 |
| rom Last In Space, a failed television pilot | Supernova produced in conjunction with the album. |
| mass of about 16-20 solar masses are type II | supernova progenitors. |
| mass of about 12-15 solar masses are type II | supernova progenitors. |
| he mass of about 12 solar masses are type II | supernova progenitors. |
| mass of about 12-16 solar masses are type II | supernova progenitors. |
| Light from the | supernova reached Earth on February 23, 1987. |
| This is believed to have been the first | supernova recorded by humankind. |
| 10, the band announced a new recorddeal with | Supernova Records/Bonnier Amigo Music Group. |
| eventh single by Orange County pop punk band | Supernova, released on 7" by Rococo Records in 2007. |
| "Costa Mesa Hates Me" is a song by | Supernova, released as their fourth single on 7" by Tr |
| second single by Orange County pop punk band | Supernova, released on 7" by Goldenrod Records in 1993 |
| an" is a song by Orange County pop punk band | Supernova, released on 7" by Sympathy for the Record I |
| The | supernova remained visible to the naked eye into 1574, |
| The Vela | supernova remnant includes NGC 2736. |
| this nebula is the brightest patch of a huge | supernova remnant (Gum Nebula) whose delicate whips co |
| central object in the | supernova remnant RX J0852.0-4622. |
| It lies close to the | supernova remnant SN 1006. |
| d, and it was shown to originate from near a | supernova remnant in the Large Magellanic Cloud. |
| reflection nebula believed to be an ancient | supernova remnant or gas cloud illuminated by nearby s |
| Supernova remnant (SNR) G315.0-02.3 has been identifie | |
| The old | supernova remnant HB 21 appears to be quite similar to |
| The association of the Vela | supernova remnant with the Vela pulsar, made by astron |
| These X-ray sources include stars, a | supernova remnant (SNR), a low-mass X-ray binary (LMXB |
| The associated | supernova remnant from this explosion was not identifi |
| The Vela | supernova remnant (SNR) is one of the closest known to |
| SNR G292.0+01.8 is | supernova remnant located in the constellation Carina. |
| idered the same source as Sct X-1 and may be | supernova remnant SNR 027.4+00.0. |
| W50 or SNR G039.7-02.0 is a | Supernova remnant located in the Aquila constellation, |
| The | supernova remnant is in Circinus and Centaurus, but th |
| 33, a star forming region that includes the | supernova remnant G337.0-0.1. |
| , Nova Cygni 1936) and parts of the extended | supernova remnant HB 21 (G89.0+4.7). |
| t-years in width and has the attributes of a | supernova remnant from an explosive event that occurre |
| It also overlaps the Puppis | Supernova Remnant, which is four times more distant. |
| It is part of the Vela | Supernova Remnant, located near the Vela Pulsar in the |
| rved from objects such as the Crab Nebula, a | supernova remnant, and Markarian 421, a blazar. |
| Tour of Tycho's | Supernova Remnant. |
| A composite image of the | supernova remnant. |
| early 1970s, the Medusa was thought to be a | supernova remnant. |
| pulsar was the first to be connected with a | supernova remnant. |
| en found which is believed to be from an old | supernova remnant. |
| om part of the shock wave of the larger Vela | Supernova Remnant. |
| eated the black hole or it was born out of a | supernova remnant. |
| tary system formation resulting from unusual | supernova remnants or a quark nova. |
| o sources were known within this region, two | supernova remnants bordered it and a known satellite g |
| Nova remnants are much less massive than | supernova remnants or planetary nebulae. |
| urces but particularly large radio galaxies, | supernova remnants and emission nebulae. |
| n, in which superbubbles of ionised gas from | supernova remnants expand vertically through galactic |
| de range of astrophysical sources, including | supernova remnants, active galactic nuclei, cataclysmi |
| HD has also been found in | Supernova remnants, and other sources. |
| he origin and evolution of neutron stars and | supernova remnants, and active galactic nuclei. |
| mainly of shocks including solar flares and | supernova remnants. |
| urces and G111.7-2.1 in the Green Catalog of | Supernova Remnants. |
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