"Red Rectangle" meaning in English

{
  "etymology_text": "Coined by astronomers Martin Cohen and Mike Merrill in 1973",
  "forms": [
    {
      "form": "the Red Rectangle",
      "tags": [
        "canonical"
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    }
  ],
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      "expansion": "the Red Rectangle",
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  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
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      "examples": [
        {
          "text": "1987, Beverly T. Lynds, “Optical observations of nebulae”, in A. Dalgarno and David Layzer (eds.), Spectroscopy of astrophysical plasmas, Cambridge University Press, →ISBN, page 12,\nThe Red Rectangle is only one example of an infrared object that is detectable in the infrared because of grain emission."
        },
        {
          "text": "1995, J.R. Miles, P.J. Sarre, and S.M. Scarrott, “Red Rectangle Emission Bands”, in Alexander G.G.M. Tielens and Theodore Peck Snow (eds.), The Diffuse Interstellar Bands, Springer, →ISBN, page 143,\nThe Red Rectangle is a bipolar nebula with a remarkable spectrum in which emission is excited by the light of the central star HD44179."
        },
        {
          "ref": "2000 July, T. Miyata et al., “Spatially Resolved Spectra of the Red Rectangle in the N-band”, in Ryszard Szczerba, Sławomir K. Górny, editors, Post-AGB as a Phase of Stellar Evolution: Proceedings of the Toruń Workshop held July 5-7, 2000, Kluwer Academic Publishers, published 2001, →ISBN, page 352:",
          "text": "Figure 1 shows obtained images of the Red Rectangle. All of the sources consist of a bright core and an extended nebula.",
          "type": "quote"
        }
      ],
      "glosses": [
        "The nebula and binary star HD 44179."
      ],
      "id": "en-Red_Rectangle-en-name-owB1BEfn",
      "links": [
        [
          "astronomy",
          "astronomy"
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      ],
      "raw_glosses": [
        "(astronomy) The nebula and binary star HD 44179."
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    }
  ],
  "word": "Red Rectangle"
}

{
  "etymology_text": "Coined by astronomers Martin Cohen and Mike Merrill in 1973",
  "forms": [
    {
      "form": "the Red Rectangle",
      "tags": [
        "canonical"
      ]
    }
  ],
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      },
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    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
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      "examples": [
        {
          "text": "1987, Beverly T. Lynds, “Optical observations of nebulae”, in A. Dalgarno and David Layzer (eds.), Spectroscopy of astrophysical plasmas, Cambridge University Press, →ISBN, page 12,\nThe Red Rectangle is only one example of an infrared object that is detectable in the infrared because of grain emission."
        },
        {
          "text": "1995, J.R. Miles, P.J. Sarre, and S.M. Scarrott, “Red Rectangle Emission Bands”, in Alexander G.G.M. Tielens and Theodore Peck Snow (eds.), The Diffuse Interstellar Bands, Springer, →ISBN, page 143,\nThe Red Rectangle is a bipolar nebula with a remarkable spectrum in which emission is excited by the light of the central star HD44179."
        },
        {
          "ref": "2000 July, T. Miyata et al., “Spatially Resolved Spectra of the Red Rectangle in the N-band”, in Ryszard Szczerba, Sławomir K. Górny, editors, Post-AGB as a Phase of Stellar Evolution: Proceedings of the Toruń Workshop held July 5-7, 2000, Kluwer Academic Publishers, published 2001, →ISBN, page 352:",
          "text": "Figure 1 shows obtained images of the Red Rectangle. All of the sources consist of a bright core and an extended nebula.",
          "type": "quote"
        }
      ],
      "glosses": [
        "The nebula and binary star HD 44179."
      ],
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        "(astronomy) The nebula and binary star HD 44179."
      ],
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        "astronomy",
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  ],
  "word": "Red Rectangle"
}