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Ontology:Q11,87: Difference between revisions

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m link: Necrozma
black hole M87 star sense-label / test tts parameter / Usage notes
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{{HueCSS}}<!--
{{HueCSS}}<ol class="hue clean compound"><li> {{ArticleTitle|black hole - STM / Z0 / Q11,87}}
--><ol class="hue clean compound"><li>
<onlyinclude><dfn class="{{{class|field_geo}}} manual" data-dimension="Z0" data-qid="1187" data-numbersign="200" data-field="" data-series="" data-work="" data-chapter="" data-tale="" data-object="" data-note="" data-lexeme="">{{IZ0}}{{#switch: {{{ParameterThatShouldAlwaysBeEmpty|}}} | {{{tts|}}}{{{1|}}} = [[E:Q1187|black hole]] | {{{tts|}}} = [[E:Q1187|{{{1}}}]] | #default = [[E:Q1187|{{TTS|tts={{{tts}}}|{{{1}}}}}]] }}{{#if: {{{3|}}} | {{{3}}} }}{{#if: {{{2|}}} | <ins class="edition-sense term"> ([[E:Q1187/{{{2}}}|{{{2}}}]]<nowiki />)</ins> }}{{WaveScore|sum=1|quilt=1|ply=1|enddfn=1}}{{#switch: {{{C|}}} | L = <span></span> | Q = <span></span> | F = [[C:Black hole physics ontology]] }}</onlyinclude>  <!-- F = physics, fízika (ru) -->
<onlyinclude><dfn class="field_geo" data-dimension="Z" data-qid="1187" data-numbersign="200" data-field="" data-series="" data-work="" data-chapter="" data-tale="" data-object="" data-note="" data-lexeme="">{{#if: {{{1|}}} | [[Ontology:{{{1}}}|{{{1}}}]] | [[Ontology:Q1187|black hole]] }}{{WaveScore|sum=1|quilt=1|ply=1}}</dfn></onlyinclude>  __NOTOC__
</li></ol><!-- duplication hint:  copy or update fake Item from [[Special:PermanentLink/NNNN|Q1187]] -->  __NOTOC__
</li></ol>


== Characteristics in draft ==
== Core characteristics ==
 
=== Properties ===


<dl class="wikitable hue">
<dl class="wikitable hue">
{{HueClaim|P=item type| {{Template:Z1}} }}
{{HueClaim |P=item type| {{Template:Z0}} }}
{{HueRoster|P=label (en)| {{Ontology:Q1187}} }}
{{HueRoster|EP=PPPA/L|lang=en| {{E:Q1187}} | {{E:Q1187/SN}} }}
{{HueClaim|P=alias (en)| -- }}
{{HueClaim |EP=PPPA|lang=en| -- }}
{{HueRoster|P={{Ontology:P42}}| -- }}  <!-- en: QID references -->
{{HueRoster|EP=P42| star catalog | M87 black hole image }}  <!-- en: QID references -->
{{HueRoster|P={{Ontology:P56}}| physics }}  <!-- en: color swatch references -->
{{HueRoster|EP=P56| physics }}  <!-- en: color swatch references -->
{{HueRoster|P=subset of| -- }}  <!-- en: subset of -->
{{HueRoster|EP=P3| -- }}  <!-- en: subset of -->
{{HueRoster|P=instance of| -- }}  <!-- en: instance of -->
{{HueRoster|EP=P4| -- }}  <!-- en: instance of -->
{{HueRoster|P=superset of| -- }}  <!-- en: superset of -->
{{HueRoster|EP=P5| -- }}  <!-- en: superset of -->
{{HueRoster|P=appears in work| -- }}  <!-- en: superset of -->
{{HueRoster|EP=P14| -- }}  <!-- en: superset of -->
{{HueClaim|P=[[User:Reversedragon/FirstNineThousand|prototype]] notes| -- }}
{{HueRoster|P=duplication hint| <code>copy or update fake Item from [[Special:PermanentLink/</code>{{REVISIONID}}<code>|Q1180]]</code> }}
</dl>
</dl>


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== Wavebuilder combinations ==
== Wavebuilder combinations ==


<dl class="wikitable hue data_wavebuild">   
<dl class="wikitable hue data_wavebuild three">   
{{WaveBuild| {{Ontology:Q8925}} | {{Ontology:Q11800}} }}  <!-- en: WITH  Pokémon  PRODUCES  Necrozma -->
{{WaveBuild| {{E:Q1187}} | {{E:Q8925}} | {{E:Q11800}} }}  <!-- en: WITH  Pokémon  PRODUCES  Necrozma -->
</dl>
</dl>


== Usage notes ==
== Usage notes ==


=== Item number ===
The "87" within the Item ID is in reference to the black hole {{TTS|tts=M87 star|M87*}}, which was the subject of the world's first black hole photograph. "M87" by itself refers to the containing galaxy, while specific black holes are sometimes given a "star" identifier in some articles to distinguish them as unique objects which can be isolated with the right kind of filter from radio signals coming out of the centers of their galaxies. <ref name="se" /> <ref name="se2" />
=== References ===
<references>
<ref name="se"><cite class="article">Why do some supermassive black holes have a * in their name?</cite>. @usernumber & contributors. (<time datetime="2022-04-18T09:40:54Z">18 April 2022</time>). Astronomy Stack Exchange. [https://astronomy.stackexchange.com/questions/49133/why-do-some-supermassive-black-holes-have-a-in-their-name]</ref>


[[Category:Black hole physics ontology]]
<ref name="se2"><cite class="article">The discovery of {{TTS|tts=Sagittarius A star|Sgr A*}}</cite>. Goss, W.M., Brown, R.L., and Lo, K.Y. (2003). <cite lang="de">Astronomische Nachrichten</cite>, 324(S1), pp. 497–504. Wiley; arxiv.org. [https://dx.doi.org/10.1002/asna.200385047 dx.doi.org] [http://arxiv.org/abs/astro-ph/0305074v1] [https://arxiv.org/abs/astro-ph/0305074]</ref>  [[Category:Examples of bop-format journal article citations]]
</references>

Revision as of 05:25, 4 August 2025

  1. pronounced [Z0] black hole 1-1-1

Core characteristics

item type
Z0 1-1-1
pronounced [P] label [string] (L)
pronounced [Z0] black hole 1-1-1
pronounced [Z0] pronounced black hole such as M87* (SN) 1-1-1
pronounced [P] alias (en) [string]
--
QID references [Item] 1-1-1
star catalog
M87 black hole image
color swatch references [Item]
physics
sub-case of [Item]
--
case of [Item]
--
super-case of [Item]
--
appears in work [Item]
--

Hypothetical models

believed to operate according to model
--

Wavebuilder combinations

pronounced [P] pronounced Wavebuilder: forms result [Item]
Necrozma (Pokémon) 1-1-1
along with [Item]
pronounced [Z0] black hole 1-1-1
forming from [Item]
pronounced [Z0] black hole 1-1-1
Pokémon (being) 1-1-1
Necrozma (Pokémon) 1-1-1

Usage notes

Item number

The "87" within the Item ID is in reference to the black hole pronounced M87*, which was the subject of the world's first black hole photograph. "M87" by itself refers to the containing galaxy, while specific black holes are sometimes given a "star" identifier in some articles to distinguish them as unique objects which can be isolated with the right kind of filter from radio signals coming out of the centers of their galaxies. [1] [2]

References

  1. Why do some supermassive black holes have a * in their name?. @usernumber & contributors. (). Astronomy Stack Exchange. [1]
  2. The discovery of pronounced Sgr A*. Goss, W.M., Brown, R.L., and Lo, K.Y. (2003). Astronomische Nachrichten, 324(S1), pp. 497–504. Wiley; arxiv.org. dx.doi.org [2] [3]