「Centaurus」の共起表現一覧(1語右で並び替え)
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| Since | Centaurus A is about 15 million light-years away from |
| Its host galaxy was | Centaurus A about 15 million light-years away in the c |
| iolet light, which comes from young stars of | Centaurus A. |
| of the dust disk in front of the nucleus of | Centaurus A. Credit: HST/NASA/ESA. |
| middle of the left part of the dust belt of | Centaurus A. The blue-green color occurs because David |
| htest galaxy within the subgroup centered on | Centaurus A. |
| 53 is located within the M83 Subgroup of the | Centaurus A/M83 Group, a relatively nearby group of ga |
| 5408 is located near the M83 Subgroup of the | Centaurus A/M83 Group, a relatively nearby group of ga |
| 945 one of the brightest galaxies within the | Centaurus A/M83 Group, a large, nearby group of galaxi |
| The border between | Centaurus and Circinus lies within the 5" radius, 95% |
| ed by pirates are the Sirius Star, the Maran | Centaurus, and the Irene SL. |
| s somewhat into the neighbour constellations | Centaurus and Musca. |
| e second brightest star in the constellation | Centaurus, and the Agena unmanned target vehicle used |
| stars in the constellations Scorpius, Lupus, | Centaurus, and Crux are members of the Sco-Cen associa |
| e second brightest star in the constellation | Centaurus and the tenth brightest star in the night sk |
| e patch of sky between the constellations of | Centaurus and Vela. |
| It lies between | Centaurus and Scorpius. |
| he Scutum Arm, then gradually turns into the | Centaurus Arm. |
| lation Lupus was a sectional asterism within | Centaurus as an unspecified animal, possibly a wolf, c |
| 107914 is a binary star in the constellation | Centaurus at ≈78.3 pc from the Sun classified as a whi |
| ed, as seen from Earth, in the constellation | Centaurus, but it is actually several thousand light y |
| on Crux (the Southern Cross) with stars from | Centaurus but these were in fact already formed (and d |
| The supernova remnant is in Circinus and | Centaurus, but the causitive X-ray source is most like |
| mber from June 2007 of the Advisory Board of | Centaurus Capital, a London based hedge fund managemen |
| The | Centaurus cluster shares its supercluster, the Hydra-C |
| The | Centaurus Cluster (A3526) is a cluster of hundreds of |
| It is the brightest galaxy in the | Centaurus Cluster, a large, rich cluster of galaxies i |
| ant a redesign by Bristol to use the Bristol | Centaurus engine. |
| Fischer is a 1992 graduate of | Centaurus High School, a 1996 graduate of the United S |
| ntury BCE and Aratus in the 3rd century BCE, | Centaurus is an ancient constellation. |
| he Centaur Oakblue or Dull Oakblue (Arhopala | centaurus) is a species of lycaenid or blue butterfly |
| During the collapse of Amaranth Advisors, | Centaurus is widely credited as being one of the major |
| Centaurus is a bright constellation in the southern sk | |
| The | Centaurus is a mixed-use development project currently |
| is, Vela, Carina, Crux (the Southern Cross), | Centaurus, Lupus, and Scorpius (including the Scorpius |
| alaxy, is located on the border of Hydra and | Centaurus, M68 is a globular cluster near M83, and M48 |
| ntually immortalized in the constellation of | Centaurus or in some versions, Sagittarius |
| Not to be confused with | Centaurus Supercluster or Centaurus A/M83 Group. |
| Centaurus: The Best of Australian Science Fiction (199 | |
| but found a 'cloud' in the constellation of | Centaurus to be the most striking concentration of gal |
| The | Centaurus under construction on 6 July, 2010. |
| devastating loss at the hands of the mighty | Centaurus Warriors. |
| ne of the largest constellations in the sky, | Centaurus was included among the 48 constellations lis |
| When Enron collapsed in 2002, he founded | Centaurus with his previous year's bonus. |
| t (SNR) G315.0-02.3 has been identified with | Centaurus X-1. |
| Centaurus X-3 was first observed during experiments of | |
| Main article: | Centaurus X-3 |
| Centaurus X-3 (4U 1118-60) is an X-ray pulsar with a p | |
| therefore evidence for the binary nature of | Centaurus X-3. |
| pe K3-K7V for a low-mass X-ray binary (LMXB) | Centaurus X-4 at about 53 amin from Cen XR-4. |
| Centaurus XR-2 on October 15, 1967, (Cen XR-2 Lewin), | |
| e visual identification for the X-ray source | Centaurus XR-2. |
| Both Cen XR-2 and | Centaurus XR-3 appeared in a position previously obser |
| mical objects within the ±2° error circle of | Centaurus XR-4. |
| ter discovery, it is subsequently designated | Centaurus XR-4. |
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