Beehive Proplyd - Revision history

YoulaAzkarrula at 04:47, 16 June 2026

2026-06-16T04:47:58Z

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	[[Category:IAU-Star Name‏‎]]		[[Category:IAU-Star Name‏‎]]
	[[Category:English]]		[[Category:English]]
	[[Category:Modern]]		[[Category:Modern]] [[Category:Asterism]] [[Category:Star Name]] [[Category:Ori]]

Sushoff at 14:58, 13 June 2026

2026-06-13T14:58:30Z

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	comparisons indicate that the Beehive proplyd quantitatively behaves like the inner region proplyds in spite of its much greater distance from θ 1Ori C and its bizarre appearance </blockquote>		comparisons indicate that the Beehive proplyd quantitatively behaves like the inner region proplyds in spite of its much greater distance from θ 1Ori C and its bizarre appearance </blockquote>The name is taken up in several papers in 2010 and 2015.

	==Mythology==		==Mythology==

Sushoff at 14:55, 13 June 2026

2026-06-13T14:55:47Z

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	==Concordance, Etymology, History==		==Concordance, Etymology, History==
	The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper by Bally+ due to its inner structure with multiple bows.<ref name=":0" /> They reason for their naming: <blockquote>The ionization front of this proplyd has a remarkable morphology not seen in any other object in Orion. The irradiated northern rim of this proplyd exhibits a set of coaxial rings centered on the axis of the outflow emerging from the young central star. These rings lie in planes roughly parallel to the orientation of the circumstellar disk surrounding the star, which is clearly seen in silhouette against background nebular light. The rings give this giant proplyd its distinctive appearance, which resembles a large beehive. </blockquote>The object itself is not visible, as it is hidden in the nebula, but as a protoplanetary disk is - by definition - surrounding a young star, there is a star inside.		The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper by Bally+ due to its inner structure with multiple bows.<ref name=":0" /> They reason for their naming: <blockquote>The ionization front of this proplyd has a remarkable morphology not seen in any other object in Orion. The irradiated northern rim of this proplyd exhibits a set of coaxial rings centered on the axis of the outflow emerging from the young central star. These rings lie in planes roughly parallel to the orientation of the circumstellar disk surrounding the star, which is clearly seen in silhouette against background nebular light. The rings give this giant proplyd its distinctive appearance, which resembles a large beehive. </blockquote>The object itself is not visible, as it is hidden in the nebula, but as a protoplanetary disk is - by definition - surrounding a young star, there is a star inside. It is classified as a high velocity object since O'Dell and Henney 2008 ('''2008AJ....136.1566O'''<ref>O'Dell, C. R. and Henney, W. J., “High Spatial Velocity Features in the Orion Nebula,”, <nowiki><i>The Astronomical Journal</i></nowiki>, vol. 136, no. 4, IOP, pp. 1566–1586, 2008. doi:10.1088/0004-6256/136/4/1566.</ref>). <blockquote> The vertical axis points toward P.A. = 355.3◦. The inner silhouette disk is discernible around the central star, as are two microjets, the lower (southern and opposite to the ionizing star θ 1Ori C) being brighter. The ripples in the ionized shell are probably caused by irregularities in the rate of mass loss within the microjets.

			(...)

			comparisons indicate that the Beehive proplyd quantitatively behaves like the inner region proplyds in spite of its much greater distance from θ 1Ori C and its bizarre appearance </blockquote>

	==Mythology==		==Mythology==

Sushoff at 14:47, 13 June 2026

2026-06-13T14:47:04Z

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	[[File:BeehiveProplyd.png\|thumb\|A large proplyd that shows a disk and rings surrounding it (Bally et al. 2005)<ref name=":0">Bally, J., Licht, D., Smith, N., and Walawender, J., “Outflows in the Orion Nebula: HH 540 from the Beehive Proplyd”, <nowiki><i>The Astronomical Journal</i></nowiki>, vol. 129, no. 1, IOP, pp. 355–362, 2005. doi:10.1086/426324.</ref>.]]		[[File:BeehiveProplyd.png\|thumb\|A large proplyd that shows a disk and rings surrounding it (Bally et al. 2005)<ref name=":0">Bally, J., Licht, D., Smith, N., and Walawender, J., “Outflows in the Orion Nebula: HH 540 from the Beehive Proplyd”, <nowiki><i>The Astronomical Journal</i></nowiki>, vol. 129, no. 1, IOP, pp. 355–362, 2005. doi:10.1086/426324.</ref>.]]
	Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the ~~star ...~~ in constellation [[Orion]].		Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the Herbig-Haro Object HH540 in constellation [[Orion]].


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	==Concordance, Etymology, History==		==Concordance, Etymology, History==
	The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper by Bally+ due to its inner structure with multiple bows.<ref name=":0" /> They reason for their naming: <blockquote>The ionization front of this proplyd has a remarkable morphology not seen in any other object in Orion. The irradiated northern rim of this proplyd exhibits a set of coaxial rings centered on the axis of the outflow emerging from the young central star. These rings lie in planes roughly parallel to the orientation of the circumstellar disk surrounding the star, which is clearly seen in silhouette against background nebular light. The rings give this giant proplyd its distinctive appearance, which resembles a large beehive. </blockquote>		The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper by Bally+ due to its inner structure with multiple bows.<ref name=":0" /> They reason for their naming: <blockquote>The ionization front of this proplyd has a remarkable morphology not seen in any other object in Orion. The irradiated northern rim of this proplyd exhibits a set of coaxial rings centered on the axis of the outflow emerging from the young central star. These rings lie in planes roughly parallel to the orientation of the circumstellar disk surrounding the star, which is clearly seen in silhouette against background nebular light. The rings give this giant proplyd its distinctive appearance, which resembles a large beehive. </blockquote>The object itself is not visible, as it is hidden in the nebula, but as a protoplanetary disk is - by definition - surrounding a young star, there is a star inside.

	==Mythology==		==Mythology==

Sushoff at 14:44, 13 June 2026

2026-06-13T14:44:40Z

← Older revision		Revision as of 14:44, 13 June 2026
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	Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation [[Orion]].		Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation [[Orion]].


			[[File:BeehiveProplyd in M42.png\|thumb\|BeehiveProplyd in M42, screenshot from Aladin]]

	==Concordance, Etymology, History==		==Concordance, Etymology, History==

Sushoff at 14:41, 13 June 2026

2026-06-13T14:41:40Z

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	Authors: {{PAGEAUTHORS}}		Authors: {{PAGEAUTHORS}}
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	[[File:~~Example~~.~~jpg~~\|thumb\|~~InfoCard1]]~~		[[File:BeehiveProplyd.png\|thumb\|A large proplyd that shows a disk and rings surrounding it (Bally et al. 2005)<ref name=":0">Bally, J., Licht, D., Smith, N., and Walawender, J., “Outflows in the Orion Nebula: HH 540 from the Beehive Proplyd”, <nowiki><i>The Astronomical Journal</i></nowiki>, vol. 129, no. 1, IOP, pp. 355–362, 2005. doi:10.1086/426324.</ref>.]]
	~~[[File~~:~~Example~~.~~jpg\|thumb\|InfoCard2~~]]
	Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation [[Orion]].		Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation [[Orion]].


	==Concordance, Etymology, History==		==Concordance, Etymology, History==
	The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper due to its inner structure with multiple bows.		The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper by Bally+ due to its inner structure with multiple bows.<ref name=":0" /> They reason for their naming: <blockquote>The ionization front of this proplyd has a remarkable morphology not seen in any other object in Orion. The irradiated northern rim of this proplyd exhibits a set of coaxial rings centered on the axis of the outflow emerging from the young central star. These rings lie in planes roughly parallel to the orientation of the circumstellar disk surrounding the star, which is clearly seen in silhouette against background nebular light. The rings give this giant proplyd its distinctive appearance, which resembles a large beehive. </blockquote>

	==Mythology==		==Mythology==

Sushoff: Created page with "Authors: {{PAGEAUTHORS}} ---- InfoCard1 InfoCard2 Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation Orion. ==Concordance, Etymology, History== The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper d..."

2026-06-13T14:37:13Z

Created page with "Authors: {{PAGEAUTHORS}} ---- thumb|InfoCard1 thumb|InfoCard2 Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation Orion. ==Concordance, Etymology, History== The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper d..."

New page

Authors: {{PAGEAUTHORS}}
----
[[File:Example.jpg|thumb|InfoCard1]]
[[File:Example.jpg|thumb|InfoCard2]]
Beehive Proplyd is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern astrophysics English. It is the name of the star ... in constellation [[Orion]].

==Concordance, Etymology, History==
The protoplanetary disk (proplyd) in the Great Orion Nebula was nicknamed "Beehive" in a 2005 paper due to its inner structure with multiple bows.

==Mythology==
no mythology

==IAU Working Group on Star Names==
The name was adopted by the IAU WGSN in 2026, as it has been in popular use among astrophysicists and listed in SIMBAD already.

<gallery>
File:Example.jpg|InfoCard1
File:Example.jpg|InfoCard2
</gallery>

== Weblinks ==

*

== Reference ==
* [[References|References (general)]]
* [[References (Medieval and Early Modern)|References (early modern)]]
* Ian Ridpath's website ([http://ianridpath.com/startales Star Tales] )

[[Category:IAU-Star Name‏‎]]
[[Category:English]]
[[Category:Modern]]