「Solar」の共起表現一覧(1語右で並び替え)8ページ目
該当件数 : 3374件
| Topray | Solar is a player in the renewable energy industry w |
| Solar is an American fictional comic book character. | |
| First | Solar is by far the world's largest thin-film solar |
| Zenith | Solar is an Israeli solar energy company based in Ne |
| Envision | Solar is also the only solar energy company to provi |
| Sundog | Solar is a solar energy company based in Chatham, NY |
| Solar is surrounded by Vendipalayam in the north, La | |
| Topray | Solar is a fully vertically integrated solar manufac |
| Solar is well known for its weekly shandy that takes | |
| Envision | Solar is the only company in the world composed of a |
| Based on its mass of 1.68 | solar, it was an A-type star when it was a main-sequ |
| In the past the building was also home to the | Solar Jackets and an aerial team. |
| of a unique codex titled Relaxatia, an ancient | Solar Kundalini paradigm that he rediscovered throug |
| an R&B group Shalamar, released in 1978 on the | SOLAR label. |
| The | Solar Laboratory was designed in the Mission Revival |
| The Hale | Solar Laboratory was the laboratory of astronomer Ge |
| Observatory, George Ellery Hale built the Hale | Solar Laboratory as his office and workshop, pursuin |
| as director at Mount Wilson, he built the Hale | Solar Laboratory in Pasadena, California, as his off |
| The Hale | Solar Laboratory is located at 740 Holladay Drive, P |
| The Hale | Solar Laboratory was declared a National Historic La |
| They are the Gamble House, the Hale | Solar Laboratory, the Rose Bowl, and two sites at th |
| Observatory, Palomar Observatory, and the Hale | Solar Laboratory. |
| nitiatives, the most significant of which is a | solar lamp programme. |
| A | solar lamp is a portable light fixture composed of a |
| Solar lamps recharge during the day. | |
| friendly luxury condos, or a project building | solar latrines to improve sanitation in Bolivia. |
| Passive | solar layout and features |
| Heliotronics of Hingham, MA provided a | Solar Learning Lab, which gives students real-time s |
| It has been replaced by a low powered | solar light in front of the original tower whose foc |
| is a codex of the human chakra system and the | solar light spectrum, designed to activate Kundalini |
| The plates absorb | solar light which is converted to fluorescence guide |
| In 1989, a Coast Guard-approved | solar light was installed in the lantern room. |
| Sun lighter and | solar lighter (in English) |
| Solar lights are used for decoration, and come in a | |
| also devoted efforts to observation of these ' | solar like' observations in other stars, a science n |
| to investigate the physical conditions of the | solar limb, particularly the chromosphere of the Sun |
| rly titled albums, see Live at Sweet Basil and | Solar: Live at Sweet Basil. |
| For the 1991 album, see | Solar: Live at Sweet Basil. |
| album of this evenings concert was released as | Solar: Live at Sweet Basil (1991). |
| ntunwonsi's Live at Sweet Basil, McCoy Tyner's | Solar: Live at Sweet Basil and the Jean-Michel Pilc |
| Solar: Live at Sweet Basil is a 1991 live album by M | |
| Solar Living Institute | |
| of also function as sunbathing areas, in which | solar louvres break up the sunlight into a dappled s |
| ass of the sun and its luminosity is about 200 | solar luminosities. |
| an effective temperature of 5705 ± 27 K and a | solar luminosity 1.28. |
| an absolute magnitude of 0.61, nearly 49 times | solar luminosity. |
| ent knowledge to be able to predict prescribed | solar, lunar and venusian events and cycles, such as |
| d geometry are very similar to the large-scale | solar magnetic field. |
| Sami K.; Stenflo, J.O. (1984), "Properties of | solar magnetic fluxtubes as revealed by Fe I lines", |
| He is a recognised authority in | Solar Magnetohydrodynamics (or MHD for short), the s |
| nelius remained good friends, and as a result, | SOLAR maintained close ties to the Soul Train show. |
| clipse is a Valiant Comics character, a foe of | Solar, Man of the Atom. |
| Originally known as Doctor | Solar, Man of the Atom, he first appeared in a comic |
| Besides penciling the popular series | Solar, Man of the Atom and Bloodshot, Perlin also ed |
| ction from 2005, becoming the most diversified | solar manufacturer in China ever since. |
| At .08 | solar mass it is near the lower mass limit for a sta |
| 23b is the second star with mass less than 0.1 | solar mass whose radius has been directly measured; |
| 0.000 003 003 | Solar mass (Ms) |
| The pulsar is about 1.8 | solar mass and the companion is about 0.25 solar mas |
| The 16th magnitude central star has about 0.7 | solar mass and the nebula itself about 0.15 solar ma |
| The planet parameters are given for the 0.71 | Solar mass B component (Muterspaugh et al. 2010). |
| The existence of this planet around a 1.68 | solar mass star provides evidence for the existence |
| The | Solar Mass Ejection Imager (SMEI) is an instrument i |
| o the white dwarf, except what remains, a 0.05 | solar mass ball, which is too small to continue fusi |
| It sent half a | solar mass to Zeta Cygni, along with the heavy chemi |
| 0.0009546 | Solar mass (Ms) |
| The | solar mass can be determined from the length of the |
| r researchers also noted that its mass, at .08 | solar mass, is right at the lower limit needed to cr |
| The mass of the companion is ~1 | solar mass, while the pulsar mass is unusually large |
| Its mass is exactly the same as our Sun, 1 | solar mass, and it is slightly larger in radius, at |
| sses "M" commonly reported as multiples of one | solar mass, |
| ompanion with putative mass that yields 70% of | Solar mass. |
| The mass would be 11% | solar mass. |
| Sargas has been determined to be 3.7 times the | solar mass. |
| the lowest mass was the star Wolf 359 at 0.09 | solar mass. |
| It has a mass of 1.33 | solar masses and a radius of 1.79 times that of our |
| ith's cloud has a mass of at least one million | solar masses and measures 3,000 parsecs (9,800 ly) l |
| nter with a rate of formation greater than 100 | solar masses per year. |
| It is approximately 1.7 | solar masses and about 3 times hotter than our Sun a |
| The ring has a mass of 100 million | solar masses and is 200,000 light years long. |
| It has 0.79 | solar masses and is a suspected variable star that v |
| parsecs was found to be between 1600 and 3200 | solar masses (95 percent confidence), consistent wit |
| le currently known to science, with a mass 3.8 | solar masses and a diameter of only 15 miles (24 kil |
| elativistic star of perhaps a hundred thousand | solar masses or larger. |
| g a merger some galaxies can make thousands of | solar masses of new stars each year, which is large |
| The original star had an estimated 5 | solar masses and was a B-type star (roughly B4-5) wh |
| One study puts the larger at 1.22 | solar masses and the smaller at 1.17, while another |
| d red supergiants with the mass of about 12-15 | solar masses are type II supernova progenitors. |
| Merope's mass is roughly 4.5 | solar masses and has a radius more than 4 times as g |
| The star has a mass of some 40 | solar masses and a surface temperature of 37,000 kel |
| Given a recent estimate of 3.7 million | solar masses for the mass of Sagittarius A* and S2's |
| He claims that 150 | solar masses is the upper limit for stars. |
| ss than the original star-remnants exceeding 5 | solar masses are produced by stars that were over 20 |
| This star has mass 0.65 | solar masses which implies that it could probably be |
| ss black hole (IMBH) with a mass of about 1300 | solar masses orbiting Sagittarius A* at a distance o |
| Stars such as this with more than 10 | solar masses are expected to end their life by explo |
| The nebula contains approximately 10 | solar masses worth of ionized gas that was ejected b |
| he precursor star is estimated to have had 200 | solar masses at the time of its formation and around |
| The explosion ejected more than 22 | solar masses of silicon and other heavy elements int |
| ting of a black hole with a mass of about 12±3 | solar masses and a late G or early K companion star |
| louds are estimated to contain about 1 million | solar masses of plasma and dust. |
| ch companion woul yield a minimum mass of 0.17 | Solar masses and be located 26.6 Astronomical Units |
| etical study shows the system started off with | solar masses of 3.0 and 2.5, but the more massive st |
| It has a total system mass of 130-200 | Solar masses and an estimated variable luminosity of |
| these objects are estimated to be around 10−4 | solar masses per year. |
| The mass of NGC 3603-A1a is 116 ± 31 | solar masses and 89 ± 16 solar masses for NGC 3603-A |
| ey et al. estimate its current mass to be 1400 | solar masses and its initial mass to be approximatel |
| the second dredge-up occur in stars with 4 - 8 | solar masses of material, when helium fusion comes t |
| ently has a mass loss rate of a few times 10−7 | solar masses per year. |
| f Sco-Cen, with masses ranging from roughly 15 | solar masses (Antares) down to below the hydrogen-bu |
| d red supergiants with the mass of about 16-20 | solar masses are type II supernova progenitors. |
| The less massive member has approximately 20 | solar masses (spectral class O8 V). |
| five brightest stars are on the order of 15-30 | solar masses in size. |
| It mass is unknown, but is probably above 8 | solar masses meaning that it will most likely explod |
| C) is a Be star with a mass of approximately 6 | solar masses and a luminosity of 1,300 times the Sun |
| A) is a Be star with a mass of approximately 7 | solar masses and a luminosity of 3,200 times the Sun |
| is a Be star with a mass of approximately 6.2 | solar masses and a luminosity of 1,600 times the Sun |
| Assuming the former, it has a mass 3.0 | solar masses and an age of 400 million years. |
| B7V which is orbited by a star of at least 0.3 | solar masses which is probably a white dwarf. |
| rved red supergiants with the mass of about 12 | solar masses are type II supernova progenitors. |
| It is a spectral type G star, about 1.16 | solar masses and radii greater than our Sun, and onl |
| d red supergiants with the mass of about 12-16 | solar masses are type II supernova progenitors. |
| riod, the known mass of the central star (1.03 | solar masses) and the amplitude of the velocity chan |
| of the Milky Way Galaxy is around 580 billion | solar masses). |
| ible mass, estimated to be around 0.07 or 0.08 | solar masses, for a hydrogen-fusing star. |
| ible mass, estimated to be around 0.07 or 0.08 | solar masses, for a hydrogen-fusing star. |
| ominant one, with a mass of approximately 1014 | solar masses, which is approximately an order of mag |
| Based on its mass of 2.4 | solar masses, it was an A-type star when it was a ma |
| The mass of RSGC1 is estimated at 30 thousand | solar masses, which makes it one the most massive op |
| suggest that a star can have at most about 120 | solar masses, but LBV 1806-20 has been measured to h |
| be the most massive on record, approaching 300 | solar masses, until it was discovered to be a binary |
| ow mass white dwarf star of approximately 0.22 | solar masses, resulting from an earlier phase of mas |
| The pair have a total mass of 1.63 | solar masses, and orbit the primary with an eccentri |
| The other object is about 0.14 | solar masses, with a radius of 5-6 solar radii. |
| The mass of RSGC3 is estimated at 20 thousand | solar masses, which makes it one the most massive op |
| mass of the third body is likely close to 0.6 | Solar masses, making the object stellar rather subst |
| xy, with an estimated mass of approximately 60 | solar masses, and is a member of the Scorpius OB1 as |
| wever, its mass is about 3.3 hundred thousands | solar masses, which means that Leo's V mass to light |
| as a bluish white B3 spectral type star of six | solar masses, with a surface temperature between 11, |
| med that this black hole had a mass of 3.8±0.5 | solar masses, which would have been the smallest fou |
| imate its age to be 4 Gyr, its mass to be 1080 | solar masses, and the number of white dwarfs to be 1 |
| vations indicate its mass is about 0.9 million | solar masses, which means that Segue's 1 mass to lig |
| low-mass white dwarf star of approximately 0.3 | solar masses, produced by a previous stage of mass t |
| rf binary companion with a likely mass of 0.05 | solar masses, every 2.01 hours. |
| For stars in the range from 0.12 to 1.0 | solar masses, M34 contains an estimated 400 members. |
| At 720 light years away and 15-17 | solar masses, it is about the same distance away fro |
| At 21.5 | solar masses, it shines with 46,000 times the Sun's |
| This happens when a stellar core above 1.44 | solar masses, the Chandrasekhar limit, collapses and |
| ar, tentatively assumed being as small as 0.19 | Solar masses, as inferred by Pribulla et al. in 2000 |
| It is a spectral type K1 or K2 giant, 1.5 - 2 | Solar masses, with an apparent magnitude of +3.32. |
| nearby Pismis 24-17 are all approximately 100 | solar masses, very large but under the stellar upper |
| B companion are 10.4±1.3, 1.8±0.2 and 8.1±1.0 | solar masses, respectively. |
| The mass is billions of | solar masses, approximately three (3) million light |
| he open cluster is estimated at 10-20 thousand | solar masses, which makes it one the most massive op |
| r second), assuming a radius of 16 km, and two | solar masses, then |
| However, its mass is about 1.5 million | solar masses, which means that Leo's mass to light r |
| primary, UScoCTIO 108A, with mass around 0.06 | solar masses, is a brown dwarf or low-mass red dwarf |
| he open cluster is estimated at 30-50 thousand | solar masses, which makes it the second most massive |
| However the mass of the galaxy-about 550,000 | solar masses-is substantial, corresponding to the ma |
| is one of the most massive stars known, at 150 | solar masses. |
| They calculated the object's mass at 4.0 x 104 | solar masses. |
| The envelope contains at least 1.4 | solar masses. |
| star is less massive at a probable mass of 30 | solar masses. |
| ck hole would have grown to about ten thousand | solar masses. |
| 00,000 Kelvin is indicated, and a mass of 0.64 | solar masses. |
| uently retracted; the more likely mass is 5-10 | solar masses. |
| een estimated to lie between 1.5 and 5 million | solar masses. |
| similar to sun with mass of approximately 1.5 | solar masses. |
| The mass of γ Pegasi is 7 to 10 | solar masses. |
| y elements and has a mass of 10 to 100 million | solar masses. |
| It has a mass of 1.25 | solar masses. |
| mperature, it must have a mass greater than 16 | solar masses. |
| It is about 0.47 | solar masses. |
| he quasar is thought to have about 500 million | solar masses. |
| lion light-years across and has a mass of 1017 | solar masses. |
| at of the Sun while it has a mass of roughly 7 | solar masses. |
| s mass is estimated to be on the order of 1015 | solar masses. |
| ii may have a mass of approximately 95% to 99% | solar masses. |
| f cluster is estimated at 2-3 hundred thousand | solar masses. |
| dividual masses are estimated at 1.07 and 0.71 | solar masses. |
| formed from a star with a mass in excess of 40 | solar masses. |
| th visual magnitude 9.66 and a mass of 0.4-0.6 | solar masses. |
| ber, of type O3 V, has an estimated mass of 45 | solar masses. |
| is a massive open cluster, with more than 500 | solar masses. |
| companion with a mass between 0.0067 and 0.030 | solar masses. |
| pernova was estimated to be in the range of 20 | solar masses. |
| dius of 26 ly (8.0 pc) and a mass of about 214 | solar masses. |
| the system could be considerably less than 130 | solar masses. |
| solar masses. | |
| as luminous as the Sun with a mass of some 20 | solar masses. |
| neutral hydrogen in it-the upper limit is 466 | solar masses. |
| Its mass is estimated to be at least 105 | Solar masses. |
| ome measurements even give the star 150 to 200 | solar masses. |
| se pairs range from three to more than a dozen | solar masses. |
| e main sequence star that had an estimated 4.4 | solar masses. |
| This star has a precise mass of 1.14552 | solar masses. |
| ee Population I stars) and between 1.5 and 2.5 | solar masses. |
| l mass of the Omega Nebula is an estimated 800 | solar masses. |
| nitude, whose mass is approximately 1.2 MΘ (in | solar masses.) |
| e, was discovered by its HI emission (5 x 10^6 | solar masses; Higdon & Wallin 2003), and appears to |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると
|
検索履歴を保存できる！
こんにちは ゲスト さん
|
ログイン |
Weblio会員(無料)になると
|
