銀河の一覧とは? わかりやすく解説

Weblio 辞書 > 辞書・百科事典 > 百科事典 > 銀河の一覧の意味・解説 

銀河の一覧

出典: フリー百科事典『ウィキペディア(Wikipedia)』 (2023/11/30 22:48 UTC 版)

以下は、著名な銀河の一覧である。


  1. ^ Local Large-Scale Structure”. Hayden Planetarium (2008年9月15日). 2008年7月28日閲覧。
  2. ^ Goldman, Stuart (2007年9月28日). “New Stars in a Galaxy's Wake”. Sky & Telescope. 2008年7月17日閲覧。
  3. ^ "Orphan' Stars Found in Long Galaxy Tail" (Press release). NASA. 20 September 2007.
  4. ^ Sun; Donahue; Voit (2007). "H-alpha tail, intracluster HII regions and star-formation: ESO137-001 in Abell 3627". arXiv:0706.1220 [astro-ph]。
  5. ^ Fraser Cain (20 September 2007). “Galaxy Leaves New Stars Behind in its Death Plunge”. Universe Today. http://www.universetoday.com/2007/09/20/galaxy-leaves-news-stars-behind-in-its-death-plunge/. 
  6. ^ Smith, Robert T. (1941). “The Radial Velocity of a Peculiar Nebula”. Publications of the Astronomical Society of the Pacific 53: 187. Bibcode1941PASP...53..187S. doi:10.1086/125301. 
  7. ^ Burbidge, E. Margaret (1964). “The Strange Extragalactic Systems: Mayall's Object and IC 883”. Astrophysical Journal 140: 1617. Bibcode1964ApJ...140.1617B. doi:10.1086/148070. 
  8. ^ Baade, W.; Minkowski, R. (1954). “On the Indentification of Radio Sources”. Astrophysical Journal 119: 215. Bibcode1954ApJ...119..215B. doi:10.1086/145813. 
  9. ^ a b c d Karen Masters (2003年12月). “Curious About Astronomy: Can any galaxies be seen with the naked eye?”. Ask an Astronomer. 2008年11月1日閲覧。
  10. ^ Magellanic Cloud”. Astronomy Knowledge Base. University of Ottawa. 2012年11月14日閲覧。
  11. ^ The Large Magellanic Cloud, LMC”. SEDS. 2012年11月14日閲覧。
  12. ^ The Small Magellanic Cloud, SMC”. SEDS. 2012年11月14日閲覧。
  13. ^ Messier 31”. SEDS. 2012年11月14日閲覧。
  14. ^ a b Black hole found in Omega Centauri”. UPI.com (2008年4月10日). 2012年12月23日閲覧。
  15. ^ John E. Bortle (2001年2月). “The Bortle Dark-Sky Scale”. Sky & Telescope. 2012年11月14日閲覧。
  16. ^ Barbara Wilson & Larry Mitchell. “The Revised AINTNO 100”. 2012年11月14日閲覧。
  17. ^ Stephen Uitti. “Farthest Naked Eye Object”. 2008年11月1日閲覧。
  18. ^ Messier 81”. SEDS. 2012年11月14日閲覧。
  19. ^ S. J. O'Meara (1998). The Messier Objects. Cambridge University Press. ISBN 0-521-55332-6 
  20. ^ Brian Skiff (1997年1月10日). “Messier 81 naked-eye”. sci.astro.amateur. 2012年11月14日閲覧。
  21. ^ Inglis, Mike. Galaxies. pp. 157-189. doi:10.1007/978-1-84628-736-7_4. 
  22. ^ Burbidge, G. (1999). “Baade & Minkowski's Identification of Radio Sources”. Astrophysical Journal 525: 569. Bibcode1999ApJ...525C.569B. 
  23. ^ SEDS, Seyfert Galaxies
  24. ^ Scientific American, "The Ghostliest Galaxies", GD Bothun, Vol. 276, No. 2, February 1997, pp.40-45, Bibcode1997SciAm.276b..40B
  25. ^ Astrophysical Journal, "Identification of the Radio Sources in Cassiopeia (A), Cygnus A, and Puppis A", Baade, W.; Minkowski, R., vol. 119, p.206, January 1954, doi:10.1086/145812 , Bibcode1954ApJ...119..206B
  26. ^ http://iopscience.iop.org/1538-3881/122/4/2055/datafile8.txt
  27. ^ Brunthaler, A.; et al. (2000). Astronomy & Astrophysics Letters 357: 45. arXiv:astro-ph/0004256. Bibcode2000A&A...357L..45B. 
  28. ^ SEDS, Lord Rosse's drawings of M51, his "Question Mark" "Spiral Nebula"
  29. ^ Ken Crosswell, "Malin 1: A Bizarre Galaxy Gets Slightly Less So", 22 January 2007
  30. ^ Annual Review of Astronomy and Astrophysics, "The Structure of Radio Galaxies", Moffet, Alan T., vol. 4, p.145, 1966, doi:10.1146/annurev.aa.04.090166.001045 , Bibcode1966ARA&A...4..145M
  31. ^ a b c Hubble, "Hubble finds a new contender for galaxy distance record", 26 January 2011
  32. ^ Sub-parsec-scale structure and evolution in Centaurus A Introduction ; Tue November 26 15:27:29 PST 1996
  33. ^ a b The 2006 Giant Flare in PKS 2155-304 and Unidentified TeV Sources
  34. ^ a b Julie McEnery. “Time Variability of the TeV Gamma-Ray Emission from Markarian 421”. Iac.es. 2008年11月1日閲覧。
  35. ^ bNet, Ablaze from afar: astronomers may have identified the most distant "blazar" yet, Sept, 2004
  36. ^ Romani; David Sowards-Emmerd; Lincoln Greenhill; Peter Michelson (2004). “Q0906+6930: The Highest-Redshift Blazar”. The Astrophysical Journal 610: L9-L11. arXiv:astro-ph/0406252. Bibcode2004ApJ...610L...9R. doi:10.1086/423201. 
  37. ^ Rodriguez Zaurin, J.; Tadhunter, C. N.; Gonzalez Delgado, R. M. (2008). “Optical spectroscopy of Arp220: the star formation history of the closest ULIRG”. Monthly Notices of the Royal Astronomical Society 384 (3): 875. arXiv:0711.0166. Bibcode2008MNRAS.384..875R. doi:10.1111/j.1365-2966.2007.12658.x. 
  38. ^ Murray, Steven (1999). “ACIS Imaging of the Starburst Galaxy M82”. Chandra Proposal ID #01700041: 362. Bibcode1999cxo..prop..362M. 
  39. ^ Starburst Galaxies: Proceedings of a Workshop (page 27) ; 2001 ; ISBN 3-540-41472-X
  40. ^ New Scientist, "Smallest galaxy hints at hidden population", David Shiga, 4 June 2007 (accessed 9 September 2010)
  41. ^ The Independent, Science & technology: WHAT ON EARTH?, 28 February 2004
  42. ^ Wired, "Astronomers Weigh Heaviest Black Hole Yet", Lisa Grossman, 12 January 2011
  43. ^ ESO Press Release 25/00 , Most Massive Spiral Galaxy Known in the Universe , 8 December 2000
  44. ^ Grebel (2000). “Star Clusters in Local Group Galaxies”. , "Massive Stellar Clusters", ASP Conf. Ser. Vol. , eds. A. Lancon & C. Boily (Provo:ASP) 2000 (211): 262-269. arXiv:astro-ph/9912529. Bibcode2000ASPC..211..262G. 
  45. ^ a b c Lehnert, M. D.; Nesvadba, N. P. H.; Cuby, J.-G.; Swinbank, A. M.; Morris, S.; Clement, B.; Evans, C. J.; Bremer, M. N. et al. (2010). “Spectroscopic confirmation of a galaxy at redshift z = 8.6”. Nature 467 (7318): 940-942. arXiv:1010.4312. Bibcode2010Natur.467..940L. doi:10.1038/nature09462. PMID 20962840. 
  46. ^ Capak, Peter; Carilli, C. L.; Lee, N.; Aldcroft, T.; Aussel, H.; Schinnerer, E.; Wilson, G. W.; Yun, M. S. et al. (2008). “Spectroscopic Confirmation of an Extreme Starburst at Redshift 4.547”. The Astrophysical Journal 681 (2): L53-L56. arXiv:0806.0657. Bibcode2008ApJ...681L..53C. doi:10.1086/590555. 
  47. ^ David R. Law, Alice E. Shapley,Charles C. Steidel, Naveen A. Reddy, Charlotte R. Christensen, Dawn K. Erb (2012年7月18日). “High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18”. Nature. 2012年7月20日閲覧。
  48. ^ Nature 443, 186-188 (14 September 2006), A galaxy at a redshift z = 6.96, doi:10.1038/nature05104;
  49. ^ a b Yoshi Taniguchi (2008). “Star Forming Galaxies at z > 5”. Proceedings of the International Astronomical Union 3. arXiv:0804.0644. doi:10.1017/S1743921308020796. 
  50. ^ a b PASJ: Publ. Astron. Soc. Japan 57, 165-182, February 25, 2005; The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6
  51. ^ a b BBC News, Most distant galaxy detected, Tuesday, 25 March 2003, 14:28 GMT
  52. ^ a b SpaceRef, Subaru Telescope Detects the Most Distant Galaxy Yet and Expects Many More, Monday, March 24, 2003
  53. ^ Kodaira; Taniguchi; Kashikawa; Kaifu; Ando; Karoji (2003). "The Discovery of Two Lyman-α Emitters Beyond Redshift 6 in the Subaru Deep Field". arXiv:astro-ph/0301096
  54. ^ New Scientist, New record for Universe's most distant object, 17:19 14 March 2002
  55. ^ BBC News, Far away stars light early cosmos, Thursday, 14 March 2002, 11:38 GMT
  56. ^ Hu, E. M.; Cowie, L. L.; McMahon, R. G.; Capak, P.; Iwamuro, F.; Kneib, J.-P.; Maihara, T.; Motohara, K. (2002). “A Redshift [CLC][ITAL]z[/ITAL][/CLC]?=-6.56 Galaxy behind the Cluster Abell 370”. The Astrophysical Journal 568 (2): L75-L79. arXiv:astro-ph/0203091. Bibcode2002ApJ...568L..75H. doi:10.1086/340424. 
  57. ^ K2.1 HCM 6A - Discovery of a redshift z = 6.56 galaxy lying behind the cluster Abell 370
  58. ^ Hu, Esther M.; McMahon, Richard G.; Cowie, Lennox L. (1999). “An Extremely Luminous Galaxy at [CLC][ITAL]z[/ITAL][/CLC] = 5.74”. The Astrophysical Journal 522: L9-L12. arXiv:astro-ph/9907079. Bibcode1999ApJ...522L...9H. doi:10.1086/312205. 
  59. ^ a b c d e f g h i j k l m n o p q r Publications of the Astronomical Society of the Pacific, 111: 1475-1502, 1999 December; SEARCH TECHNIQUES FOR DISTANT GALAXIES; INTRODUCTION
  60. ^ a b New York Times, Peering Back in Time, Astronomers Glimpse Galaxies Aborning, October 20, 1998
  61. ^ a b Astronomy Picture of the Day, A Baby Galaxy, March 24, 1998
  62. ^ a b Arjun Dey; Hyron Spinrad; Daniel Stern; Graham; Chaffee (1998). "A Galaxy at z=5.34". arXiv:astro-ph/9803137
  63. ^ a b A New Most Distant Object: z = 5.34
  64. ^ Franx, Marijn; Illingworth, Garth D.; Kelson, Daniel D.; Van Dokkum, Pieter G.; Tran, Kim-Vy (1997). “A Pair of Lensed Galaxies at [CLC][ITAL]z[/ITAL][/CLC] = 4.92 in the Field of CL 1358+62”. The Astrophysical Journal 486 (2): L75-L78. arXiv:astro-ph/9704090. Bibcode1997ApJ...486L..75F. doi:10.1086/310844. 
  65. ^ Astronomy Picture of the Day, Behind CL1358+62: A New Farthest Object, July 31, 1997
  66. ^ a b c d e "Astrophysics and Space Science" 1999, 269/270, 165-181 ; GALAXIES AT HIGH REDSHIFT - 8. Z > 5 GALAXIES ; Garth Illingworth
  67. ^ Wil van Breugel; Carlos De Breuck; Adam Stanford; Huub Rottgering; George Miley; Daniel Stern; Dante Minniti; Chris Carilli (1999). "Ultra-Steep Spectrum Radio Galaxies at Hy Redshifts". arXiv:astro-ph/9910311
  68. ^ a b Hyron Spinrad; Arjun Dey; Graham (1995). “Keck Observations of the Most Distant Galaxy: 8C1435+63 at z=4.25”. The Astrophysical Journal 438: L51. arXiv:astro-ph/9411007. Bibcode1995ApJ...438L..51S. doi:10.1086/187713. 
  69. ^ a b New Scientist, Galaxy hunters close to the edge, 5 November 1994
  70. ^ Miley, G. K.; Chambers, K. C.; van Breugel, W. J. M.; Macchetto, F. (1992). “Hubble Space Telescope imaging of distant galaxies - 4C 41.17 at Z = 3.8”. Astrophysical Journal 401: L69. Bibcode1992ApJ...401L..69M. doi:10.1086/186673. 
  71. ^ a b Chambers, K. C.; Miley, G. K.; van Breugel, W. J. M. (1990). “4C 41.17 - A radio galaxy at a redshift of 3.8”. Astrophysical Journal 363: 21. Bibcode1990ApJ...363...21C. doi:10.1086/169316. 
  72. ^ Science News, Farthest galaxy is cosmic question - 0902+34 April 23, 1988
  73. ^ Science News, Two distant galaxies provide new puzzles - 4c 41.17, B2 09021+34, November 14, 1992
  74. ^ Paola Mazzei; Gianfranco De Zotti (1995). "Dust in High Redshift Radio Galaxies and the Early Evolution of Spheroidal Galaxies". arXiv:astro-ph/9509108
  75. ^ Le Fevre, O.; Hammer, F.; Nottale, L.; Mazure, A.; Christian, C. (1988). “Peculiar morphology of the high-redshift radio galaxies 3C 13 and 3C 256 in subarcsecond seeing”. Astrophysical Journal 324: L1. Bibcode1988ApJ...324L...1L. doi:10.1086/185078. 
  76. ^ a b Lilly, S. J.; Longair, M. S. (1984). “Stellar populations in distant radio galaxies”. Royal Astronomical Society 211: 833. Bibcode1984MNRAS.211..833L. 
  77. ^ Longair, M. S. (1984). “The Most Distant Galaxies”. Journal of the British Astronomical Association 94: 97. Bibcode1984JBAA...94...97L. 
  78. ^ . Bibcode1983S&T....65..321S. 
  79. ^ Smith, H. E.; Junkkarinen, V. T.; Spinrad, H.; Grueff, G.; Vigotti, M. (1979). “Spectrophotometry of three high-redshift radio galaxies - 3C 6.1, 3C 265, and 3C 352”. The Astrophysical Journal 231: 307. Bibcode1979ApJ...231..307S. doi:10.1086/157194. 
  80. ^ The Discovery of Radio Galaxies and Quasars
  81. ^ McCarthy, P J (1993). “High Redshift Radio Galaxies”. Annual Review of Astronomy and Astrophysics 31: 639-688. Bibcode1993ARA&A..31..639M. doi:10.1146/annurev.aa.31.090193.003231. 
  82. ^ a b c Sandage, Allan (1961). “The Ability of the 200-INCH Telescope to Discriminate Between Selected World Models”. Astrophysical Journal 133: 355. Bibcode1961ApJ...133..355S. doi:10.1086/147041. 
  83. ^ Hubble, E. P. (1953). “The law of red shifts (George Darwin Lecture)”. Monthly Notices of the Royal Astronomical Society 113: 658. Bibcode1953MNRAS.113..658H. 
  84. ^ OBSERVATIONAL TESTS OF WORLD MODELS; 6.1. Local Tests for Linearity of the Redshift-Distance Relation ; Annu. Rev. Astron. Astrophys. 1988. 26: 561-630
  85. ^ Humason, M. L.; Mayall, N. U.; Sandage, A. R. (1956). “Redshifts and magnitudes of extragalactic nebulae”. Astron. J. 61: 97. Bibcode1956AJ.....61...97H. doi:10.1086/107297. 
  86. ^ a b c “1053 May 8 meeting of the Royal Astronomical Society”. The Observatory 73: 97. (1953). Bibcode1953Obs....73...97.. 
  87. ^ Merrill, Paul W. (1958). “From Atoms to Galaxies”. Astronomical Society of the Pacific Leaflets 7: 393. Bibcode1958ASPL....7..393M. 
  88. ^ Bolton, J. G. (1969). “Extragalactic Radio Sources”. Astronomical Journal 74: 131. Bibcode1969AJ.....74..131B. doi:10.1086/110786.  A&AAid:AAA001.141.093
  89. ^ a b Humason, M. L. (1936). “The Apparent Radial Velocities of 100 Extra-Galactic Nebulae”. Astrophysical Journal 83: 10. Bibcode1936ApJ....83...10H. doi:10.1086/143696. 
  90. ^ THE FIRST 50 YEARS AT PALOMAR: 1949-1999 ; The Early Years of Stellar Evolution, Cosmology, and High-Energy Astrophysics; 5.2.1. The Mount Wilson Years ; Annu. Rev. Astron. Astrophys. 1999. 37: 445-486
  91. ^ a b Chant, C. A. (1932). “Notes and Queries (Doings at Mount Wilson-Ritchey's Photographic Telescope-Infra-red Photographic Plates)”. Journal of the Royal Astronomical Society of Canada 26: 180. Bibcode1932JRASC..26..180C. 
  92. ^ Humason, Milton L. (1931). “Apparent Velocity-Shifts in the Spectra of Faint Nebulae”. Astrophysical Journal 74: 35. Bibcode1931ApJ....74...35H. doi:10.1086/143287. 
  93. ^ Hubble, Edwin; Humason, Milton L. (1931). “The Velocity-Distance Relation among Extra-Galactic Nebulae”. Astrophysical Journal 74: 43. Bibcode1931ApJ....74...43H. doi:10.1086/143323. 
  94. ^ a b Humason, M. L. (1931). “The Large Apparent Velocities of Extra-Galactic Nebulae”. Astronomical Society of the Pacific Leaflets 1: 149. Bibcode1931ASPL....1..149H. 
  95. ^ Humason, M. L. (1930). “The Rayton short-focus spectrographic objective”. Astrophys. J. 71: 351. Bibcode1930ApJ....71..351H. doi:10.1086/143255. 
  96. ^ a b c d Trimble, Virginia (1996). “H_0: The Incredible Shrinking Constant, 1925-1975”. Publications of the Astronomical Society of the Pacific 108: 1073. Bibcode1996PASP..108.1073T. doi:10.1086/133837. 
  97. ^ “The Berkeley Meeting of the Astronomical Society of the Pacific, June 20-21, 1929”. Publications of the Astronomical Society of the Pacific 41: 244. (1929). Bibcode1929PASP...41..244.. doi:10.1086/123945. 
  98. ^ a b From the Proceedings of the National Academy of Sciences; Volume 15 : March 15, 1929 : Number 3 ; THE LARGE RADIAL VELOCITY OF N. G. C. 7619 ; January 17, 1929
  99. ^ THE JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA / JOURNAL DE LA SOCIETE ROYALE D'ASTRONOMIE DU CANADA; Vol. 83, No.6 December 1989 Whole No. 621 ; EDWIN HUBBLE 1889-1953
  100. ^ a b National Academy of Sciences; Biographical Memoirs: V. 52 - VESTO MELVIN SLIPHER; ISBN 0-309-03099-4
  101. ^ Bailey, S. I. (1920). “Comet Skjellerup”. Harvard College Observatory Bulletin No. 739 739: 1. Bibcode1920BHarO.739....1B. 
  102. ^ New York Times, DREYER NEBULA NO. 584 INCONCEIVABLY DISTANT; Dr. Slipher Says the Celestial Speed Champion Is 'Many Millions of Light Years' Away. ; January 19, 1921, Wednesday
  103. ^ a b New York Times, NEBULA DREYER BREAKS ALL SKY SPEED RECORDS; Portion of the Constellation of Cetus Is Rushing Along at Rate of 1,240 Miles a Second. ; January 18, 1921, Tuesday
  104. ^ New Scientist, Baby galaxies sighted at dawn of universe, 22:34 10 July 2007
  105. ^ Lawrence Livermore National Laboratory, Lab scientists revoke status of space object
  106. ^ Hsiao-Wen Chen; Lanzetta; Sebastian Pascarelle; Noriaki Yahata (2000). "The Unusual Spectral Energy Distribution of a Galaxy Previously Reported to be at Redshift 6.68". arXiv:astro-ph/0011558
  107. ^ BBC News, Hubble spies most distant object, Thursday, April 15, 1999
  108. ^ Hu; McMahon (1996). “Detection of Lyman-alpha Emitting Galaxies at Redshift z=4.55”. Nature 382 (6588): 231-233. arXiv:astro-ph/9606135. Bibcode1996Natur.382..231H. doi:10.1038/382231a0. 
  109. ^ 31/01/02 ; DAZLE NEAR IR NARROW BAND IMAGER (PDF, 570 KB)  ; DAZLE-IoA-Doc-0002
  110. ^ ESO Press Release 11/95, ESO Astronomers Detect a Galaxy at the Edge of the Universe, 15 September 1995
  111. ^ New Scientist, Trouble at the edge of time, 21 October 1995
  112. ^ Wampler, E. J.; et al. (1996). Astronomy & Astrophysics 316: 33. arXiv:astro-ph/9512084. Bibcode1996A&A...316...33W. 
  113. ^ Elston, Richard; Bechtold, Jill; Hill, Gary J.; Ge, Jian (1996). “A Redshift 4.38 MG II Absorber toward BR 1202-0725”. Astrophysical Journal Letters v.456 456: L13. Bibcode1996ApJ...456L..13E. doi:10.1086/309853. 
  114. ^ Smail, I.; Ellis, R. S.; Aragon-Salamanca, A.; Soucail, G.; Mellier, Y.; Giraud, E. (1993). “The Nature of Star Formation in Lensed Galaxies at High Redshift”. R.a.s. Monthly Notices V.263 263: 628. Bibcode1993MNRAS.263..628S. 
  115. ^ Gravitational Lenses II: Galaxy Clusters as Lenses
  116. ^ Djorgovski, S.; Strauss, Michael A.; Spinrad, Hyron; McCarthy, Patrick; Perley, R. A. (1987). “A galaxy at a redshift of 3.215 - Further studies of the PKS 1614+051 system”. Astronomical Journal (ISSN 0004-6256) 93: 1318. Bibcode1987AJ.....93.1318D. doi:10.1086/114414. 
  117. ^ NED, Searching NED for object "3C 123"
  118. ^ Spinrad, H. (1975). “3C 123: a distant first-ranked cluster galaxy at z = 0.637”. Astrophys. J. 199: L3. Bibcode1975ApJ...199L...3S. doi:10.1086/181835. 
  119. ^ Chandra X-Ray Observatory at Havard, "Abell 644 and SDSS J1021+1312: How Often do Giant Black Holes Become Hyperactive?", 20 December 2010 (accessed 7 July 2012)
  120. ^ Sky and Telescope, Stars in the Middle of Nowhere, 10 January 2008
  121. ^ Sky and Telescope, Galaxy Monster Mash, 9 August 2007
  122. ^ ABC News, Found! Oldest galaxy pile-up, Wednesday, 9 April 2008
  123. ^ Cooke, Jeff; Barton, Elizabeth J.; Bullock, James S.; Stewart, Kyle R.; Wolfe, Arthur M. (2008). “A Candidate Brightest Protocluster Galaxy atz= 3.03”. The Astrophysical Journal 681 (2): L57-L60. arXiv:0803.3808. Bibcode2008ApJ...681L..57C. doi:10.1086/590406. 





英和和英テキスト翻訳>> Weblio翻訳
英語⇒日本語日本語⇒英語
  

辞書ショートカット

すべての辞書の索引

「銀河の一覧」の関連用語

銀河の一覧のお隣キーワード
検索ランキング

   

英語⇒日本語
日本語⇒英語
   



銀河の一覧のページの著作権
Weblio 辞書 情報提供元は 参加元一覧 にて確認できます。

   
ウィキペディアウィキペディア
All text is available under the terms of the GNU Free Documentation License.
この記事は、ウィキペディアの銀河の一覧 (改訂履歴)の記事を複製、再配布したものにあたり、GNU Free Documentation Licenseというライセンスの下で提供されています。 Weblio辞書に掲載されているウィキペディアの記事も、全てGNU Free Documentation Licenseの元に提供されております。

©2024 GRAS Group, Inc.RSS