User:Tohline/DissertationTopics/GCFormation - Revision history

Tohline: /* Centaurus A (NGC5128) */

2021-04-23T16:52:44Z

Centaurus A (NGC5128)

← Older revision		Revision as of 16:52, 23 April 2021
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	===Centaurus A (NGC5128)===		===Centaurus A (NGC5128)===

	* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''		* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy, 1 April)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''
	* NASA publicity:   (April 8, 2021) "[https://www.nasa.gov/feature/galactic-merger-warps-magnetic-fields Galactic Merger Warps Magnetic Fields]."		* NASA publicity:   (April 8, 2021) "[https://www.nasa.gov/feature/galactic-merger-warps-magnetic-fields Galactic Merger Warps Magnetic Fields]."

Tohline: /* SOFIA's Mapping of Magnetic-Field Distribution in Galaxies circa 2020 */

2021-04-23T00:52:28Z

SOFIA's Mapping of Magnetic-Field Distribution in Galaxies circa 2020

← Older revision		Revision as of 00:52, 23 April 2021
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	I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.		I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.

	==SOFIA's Mapping of Magnetic-Field Distribution in Galaxies ''circa'' ~~2020~~==		==SOFIA's Mapping of Magnetic-Field Distribution in Galaxies ''circa'' 2021==

	The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.		The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.

Tohline: /* Centaurus A (NGC 5128) */

2021-04-23T00:52:05Z

Centaurus A (NGC 5128)

← Older revision		Revision as of 00:52, 23 April 2021
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	The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.		The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.
	===Centaurus A (~~NGC 5128~~)===		===Centaurus A (NGC5128)===

	* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''		* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''

Tohline: /* Centaurus A */

2021-04-23T00:51:37Z

Centaurus A

← Older revision		Revision as of 00:51, 23 April 2021
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	The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.		The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.
	===Centaurus A===		===Centaurus A (NGC 5128)===

	* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''		* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''

Tohline: /* M51 and NGC5195 */

2021-04-23T00:49:20Z

M51 and NGC5195

← Older revision		Revision as of 00:49, 23 April 2021
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	* Archival publication:   ''not yet available''		* Archival publication:   ''not yet available''
	* NASA publicity:   (January 14, 2021) "[https://www.nasa.gov/feature/magnetic-chaos-hidden-within-the-whirlpool-galaxy Magnetic Chaos Hidden Within the Whirlpool Galaxy]."		* NASA publicity:   (January 14, 2021) "[https://www.nasa.gov/feature/magnetic-chaos-hidden-within-the-whirlpool-galaxy Magnetic Chaos Hidden Within the Whirlpool Galaxy]."
	* Sky & Telescope highlight:   M. Young (2021, May, Vol. 141, No. 5, p. 11), "Magnetic Whirlpool."		* Sky & Telescope highlight:   [https://skyandtelescope.org/astronomy-news/this-week-in-astronomy-pictures/ M. Young (2021, May, Vol. 141, No. 5, p. 11)], "Magnetic Whirlpool."
	* Related archival publication:   [https://ui.adsabs.harvard.edu/abs/2018ApJ...869L..30P/abstract J. L. Pineda ''et al.'' (2018, Astrophysical Journal Letters, 869, L30)], ''A SOFIA Survey of [C II] in the Galaxy M51. I. [CII] as a Tracer of Star Formation.''		* Related archival publication:   [https://ui.adsabs.harvard.edu/abs/2018ApJ...869L..30P/abstract J. L. Pineda ''et al.'' (2018, Astrophysical Journal Letters, 869, L30)], ''A SOFIA Survey of [C II] in the Galaxy M51. I. [CII] as a Tracer of Star Formation.''

Tohline: /* See Also */

2021-04-23T00:19:12Z

Tohline: /* SOFIA's Mapping of Magnetic-Field Distribution in Galaxies circa 2020 */

2021-04-23T00:11:43Z

SOFIA's Mapping of Magnetic-Field Distribution in Galaxies circa 2020

← Older revision		Revision as of 00:11, 23 April 2021
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	===Centaurus A===		===Centaurus A===

	~~See~~ [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''		* Archival publication:  [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''
			* NASA publicity:   (April 8, 2021) "[https://www.nasa.gov/feature/galactic-merger-warps-magnetic-fields Galactic Merger Warps Magnetic Fields]."

			===M51 and NGC5195===

			* Archival publication:   ''not yet available''
			* NASA publicity:   (January 14, 2021) "[https://www.nasa.gov/feature/magnetic-chaos-hidden-within-the-whirlpool-galaxy Magnetic Chaos Hidden Within the Whirlpool Galaxy]."
			* Sky & Telescope highlight:   M. Young (2021, May, Vol. 141, No. 5, p. 11), "Magnetic Whirlpool."
			* Related archival publication:   [https://ui.adsabs.harvard.edu/abs/2018ApJ...869L..30P/abstract J. L. Pineda ''et al.'' (2018, Astrophysical Journal Letters, 869, L30)], ''A SOFIA Survey of [C II] in the Galaxy M51. I. [CII] as a Tracer of Star Formation.''

	=See Also=		=See Also=

Tohline at 23:41, 22 April 2021

2021-04-22T23:41:50Z

← Older revision		Revision as of 23:41, 22 April 2021
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	==SOFIA's Mapping of Magnetic-Field Distribution in Galaxies ''circa'' 2020==		==SOFIA's Mapping of Magnetic-Field Distribution in Galaxies ''circa'' 2020==

	The following research efforts are very likely relevant to the idea presented above regarding the formation of globular clusters in interacting galaxies.		The following research efforts are very likely relevant to the [[#Idea_Proposed_circa_2000\|idea presented above]] regarding the formation of globular clusters in interacting galaxies.
	===Centaurus A===		===Centaurus A===

Tohline at 23:40, 22 April 2021

2021-04-22T23:40:27Z

← Older revision		Revision as of 23:40, 22 April 2021
Line 45:		Line 45:
	I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.		I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.

	==SOFIA's Mapping of Magnetic-Field in ~~M51 and~~		==SOFIA's Mapping of Magnetic-Field Distribution in Galaxies ''circa'' 2020==

			The following research efforts are very likely relevant to the idea presented above regarding the formation of globular clusters in interacting galaxies.
			===Centaurus A===

			See [https://doi.org/10.1038/s41550-021-01329-9 E. Lpez-Rodriguez (2021, Nature Astronomy)], ''The Magnetic Field Across the Molecular Warped Disk of Centaurus A.''

	=See Also=		=See Also=

Tohline at 22:40, 22 April 2021

2021-04-22T22:40:30Z

← Older revision		Revision as of 22:40, 22 April 2021
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	* [http://www.vistrails.org/images/GlobularClusterReferee.report.txt Referee Report] (received August, 2000).		* [http://www.vistrails.org/images/GlobularClusterReferee.report.txt Referee Report] (received August, 2000).
	I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.		I considered the referee's request to be well beyond the scope and essential purpose of this paper. I remain firmly convinced that the idea has a great deal of merit. I offer the original manuscript as a foundation on which an appropriately qualified graduate student might build a more extensive demonstration of the viability of this proposed mechanism for globular cluster formation.

			==SOFIA's Mapping of Magnetic-Field in M51 and

	=See Also=		=See Also=

← Older revision		Revision as of 00:19, 23 April 2021
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	* [http://adsabs.harvard.edu/abs/2015ApJ...806...35J K. E. Johnson ''et al.'' (2015, ApJ, 806, id. 35)], ''The Physical Conditions in a Pre-super Star Cluster Molecular Cloud in the Antennae Galaxies''.		* [http://adsabs.harvard.edu/abs/2015ApJ...806...35J K. E. Johnson ''et al.'' (2015, ApJ, 806, id. 35)], ''The Physical Conditions in a Pre-super Star Cluster Molecular Cloud in the Antennae Galaxies''.
			* [https://ui.adsabs.harvard.edu/abs/2020ApJ...902...28R/abstract W. T. Reach, D. Fadda, R. J. Rand, & G. J. Stacey (2020, ApJ, 902, 28)], ''Extraplanar Gas in Edge-on Galaxies Traced by SOFIA Observations of [C II]''


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