"supervirial" meaning in All languages combined

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "super",
        "3": "virial"
      },
      "expansion": "super- + virial",
      "name": "prefix"
    }
  ],
  "etymology_text": "From super- + virial.",
  "head_templates": [
    {
      "args": {
        "1": "-"
      },
      "expansion": "supervirial (not comparable)",
      "name": "en-adj"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "adj",
  "senses": [
    {
      "categories": [
        {
          "kind": "other",
          "name": "English entries with incorrect language header",
          "parents": [
            "Entries with incorrect language header",
            "Entry maintenance"
          ],
          "source": "w"
        },
        {
          "kind": "other",
          "name": "English terms prefixed with super-",
          "parents": [],
          "source": "w"
        },
        {
          "kind": "other",
          "name": "Pages with 1 entry",
          "parents": [],
          "source": "w"
        },
        {
          "kind": "topical",
          "langcode": "en",
          "name": "Physics",
          "orig": "en:Physics",
          "parents": [
            "Sciences",
            "All topics",
            "Fundamental"
          ],
          "source": "w"
        }
      ],
      "examples": [
        {
          "ref": "2008, Johan Hendrik Knapen, T. J. Mahoney, Alexandre Vazdekis, Pathways Through an Eclectic Universe, page 6:",
          "text": "For example, the 0.5-2 Myr old Orion Nebula Cluster ( ONC ), which is known to be supervirial with a virial mass about twice the observed mass ( Hillenbrand & Hartmann 1998 ), has already expelled its residual gas and is expanding rapidly.",
          "type": "quote"
        },
        {
          "ref": "2010, Mark Gieles, “Star Cluster Disruption”, in Richard de Grijs, Jacques R. D. Lépine, editors, Star Clusters (IAU S266): Basic Galactic Building Blocks, page 75:",
          "text": "For many of the young (~10Myr) star clusters M_(dyn) >> Mₚₕₒₜ Goodwin & Bastian (2006) suggest that this is a signature of gas expulsion and the 'infant mortality' scenario discussed in Section 2.1, i.e., they conclude that these clusters are supervirial.",
          "type": "quote"
        },
        {
          "ref": "2016, Richard J. Parker, Nicholas J. Wright, “Dynamical evolution of star forming regions - II. Basic kinematics”, in arXiv:",
          "text": "If measured early enough (#x3C;2 Myr in our simulations, or #x5C;sim20 crossing times), the velocity dispersion can be used to determine whether a region was highly supervirial at birth without the risk of degeneracy.",
          "type": "quote"
        },
        {
          "ref": "2019, Roberto A. Capuzzo Dolcetta, Classical Newtonian Gravity:, page 57:",
          "text": "It is subvirial when Q < 1, which corresponds to a negative acceleration of the polar inertia moment, Ï < 0 (initial contraction) and supervirial when Q >1, which corresponds to a positive acceleration of the polar inertia moment, Ï > 0 (initial expansion).",
          "type": "quote"
        }
      ],
      "glosses": [
        "Expanding at an accelerating rate."
      ],
      "id": "en-supervirial-en-adj-DLG1PrNY",
      "links": [
        [
          "physics",
          "physics"
        ],
        [
          "Expanding",
          "expand"
        ],
        [
          "accelerating",
          "accelerate"
        ]
      ],
      "raw_glosses": [
        "(physics) Expanding at an accelerating rate."
      ],
      "tags": [
        "not-comparable"
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ]
    }
  ],
  "word": "supervirial"
}

{
  "etymology_templates": [
    {
      "args": {
        "1": "en",
        "2": "super",
        "3": "virial"
      },
      "expansion": "super- + virial",
      "name": "prefix"
    }
  ],
  "etymology_text": "From super- + virial.",
  "head_templates": [
    {
      "args": {
        "1": "-"
      },
      "expansion": "supervirial (not comparable)",
      "name": "en-adj"
    }
  ],
  "lang": "English",
  "lang_code": "en",
  "pos": "adj",
  "senses": [
    {
      "categories": [
        "English adjectives",
        "English entries with incorrect language header",
        "English lemmas",
        "English terms prefixed with super-",
        "English terms with quotations",
        "English uncomparable adjectives",
        "Pages with 1 entry",
        "en:Physics"
      ],
      "examples": [
        {
          "ref": "2008, Johan Hendrik Knapen, T. J. Mahoney, Alexandre Vazdekis, Pathways Through an Eclectic Universe, page 6:",
          "text": "For example, the 0.5-2 Myr old Orion Nebula Cluster ( ONC ), which is known to be supervirial with a virial mass about twice the observed mass ( Hillenbrand & Hartmann 1998 ), has already expelled its residual gas and is expanding rapidly.",
          "type": "quote"
        },
        {
          "ref": "2010, Mark Gieles, “Star Cluster Disruption”, in Richard de Grijs, Jacques R. D. Lépine, editors, Star Clusters (IAU S266): Basic Galactic Building Blocks, page 75:",
          "text": "For many of the young (~10Myr) star clusters M_(dyn) >> Mₚₕₒₜ Goodwin & Bastian (2006) suggest that this is a signature of gas expulsion and the 'infant mortality' scenario discussed in Section 2.1, i.e., they conclude that these clusters are supervirial.",
          "type": "quote"
        },
        {
          "ref": "2016, Richard J. Parker, Nicholas J. Wright, “Dynamical evolution of star forming regions - II. Basic kinematics”, in arXiv:",
          "text": "If measured early enough (#x3C;2 Myr in our simulations, or #x5C;sim20 crossing times), the velocity dispersion can be used to determine whether a region was highly supervirial at birth without the risk of degeneracy.",
          "type": "quote"
        },
        {
          "ref": "2019, Roberto A. Capuzzo Dolcetta, Classical Newtonian Gravity:, page 57:",
          "text": "It is subvirial when Q < 1, which corresponds to a negative acceleration of the polar inertia moment, Ï < 0 (initial contraction) and supervirial when Q >1, which corresponds to a positive acceleration of the polar inertia moment, Ï > 0 (initial expansion).",
          "type": "quote"
        }
      ],
      "glosses": [
        "Expanding at an accelerating rate."
      ],
      "links": [
        [
          "physics",
          "physics"
        ],
        [
          "Expanding",
          "expand"
        ],
        [
          "accelerating",
          "accelerate"
        ]
      ],
      "raw_glosses": [
        "(physics) Expanding at an accelerating rate."
      ],
      "tags": [
        "not-comparable"
      ],
      "topics": [
        "natural-sciences",
        "physical-sciences",
        "physics"
      ]
    }
  ],
  "word": "supervirial"
}