"Red Rectangle" meaning in All languages combined

{
  "etymology_text": "Coined by astronomers Martin Cohen and Mike Merrill in 1973",
  "forms": [
    {
      "form": "the Red Rectangle",
      "tags": [
        "canonical"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {
        "def": "1",
        "head": "Red Rectangle"
      },
      "expansion": "the Red Rectangle",
      "name": "en-proper noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
  "senses": [
    {
      "categories": [
        {
          "kind": "other",
          "name": "English entries with incorrect language header",
          "parents": [
            "Entries with incorrect language header",
            "Entry maintenance"
          ],
          "source": "w"
        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Astronomy",
          "orig": "en:Astronomy",
          "parents": [
            "Sciences",
            "Space",
            "All topics",
            "Nature",
            "Fundamental"
          ],
          "source": "w"
        }
      ],
      "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, 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": "quotation"
        }
      ],
      "glosses": [
        "The nebula and binary star HD 44179."
      ],
      "id": "en-Red_Rectangle-en-name-owB1BEfn",
      "links": [
        [
          "astronomy",
          "astronomy"
        ]
      ],
      "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"
      ]
    }
  ],
  "head_templates": [
    {
      "args": {
        "def": "1",
        "head": "Red Rectangle"
      },
      "expansion": "the Red Rectangle",
      "name": "en-proper noun"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "name",
  "senses": [
    {
      "categories": [
        "English entries with incorrect language header",
        "English lemmas",
        "English multiword terms",
        "English proper nouns",
        "English terms with quotations",
        "English uncountable nouns",
        "en:Astronomy"
      ],
      "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, 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": "quotation"
        }
      ],
      "glosses": [
        "The nebula and binary star HD 44179."
      ],
      "links": [
        [
          "astronomy",
          "astronomy"
        ]
      ],
      "raw_glosses": [
        "(astronomy) The nebula and binary star HD 44179."
      ],
      "topics": [
        "astronomy",
        "natural-sciences"
      ]
    }
  ],
  "word": "Red Rectangle"
}