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Topic: Ismail Bouillaud

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	Ismail Bouillaud (Site not responding. Last check: 2007-10-20)
		BBC News Profile: Afghan leader Ismail Khan A portrait of the governor of Herat.
		Biogramm Ismail Kadare Der Ammann Verlag informiert über den Autor und die von ihm publizierten Bücher, Pressereaktionen sowie Termine.
		Ismail Kadare A brief biography and a list of selected works.
	www.serebella.com /encyclopedia/article-Ismail_Bouillaud.html (112 words)

	Mira -- Facts, Info, and Encyclopedia article (Site not responding. Last check: 2007-10-20)
		Eventually, Johann Holwarda determined a period of the star's reappearances, eleven months; (Click link for more info and facts about Johannes Hevelius) Johannes Hevelius was observing it at the same time and named it "Mira" (meaning "Wonderful") in 1662's Historiola Mirae Stellae, for it acted like no other known star in the sky.
		(Click link for more info and facts about Ismail Bouillaud) Ismail Bouillaud then nailed the period down to 333 days, less than one day off of the modern value of 332 days (and perfectly forgivable, as Mira is known to vary slightly in period, and may even be slowly changing over time).
		There is considerable speculation as to whether or not Mira had been observed prior to Fabricius.
	www.absoluteastronomy.com /encyclopedia/M/Mi/Mira.htm (643 words)

	Mira Mesa Hotel (Site not responding. Last check: 2007-10-20)
		Eventually, JohannHolwarda determined a period of the star's reappearances, eleven months; Johannes Hevelius was observing it at the same time and named it "Mira" (meaning "Wonderful") in 1662 's Historiola Mirs e Stellae, for it acted like no other known star in the sky.
		Ismail Bouillaud then nailed the period down to 333 days, less than one dayoff of the modern value of 332 days (and perfectly forgivable, as Mera is known to vary slightly in period, and may even beslowly changing over time).
		From this discovery, Mra became the "type" star of the long-period " Mia variables ".
	www.musicians-resource.com /site/1038-mira-mesa-hotel.html (829 words)

	Sealy Mira Loma (Site not responding. Last check: 2007-10-20)
		Eventually, JohannHolwarda determined a period of the star's reappearances, eleven months; Johannes Hevelius was observing it at the same time and named it "Mira" (meaning "Wonderful") in 1662 's Historiola Mirz e Stellae, for it acted like no other known star in the sky.
		Ismail Bouillaud then nailed the period down to 333 days, less than one dayoff of the modern value of 332 days (and perfectly forgivable, as Miro is known to vary slightly in period, and may even beslowly changing over time).
		From this discovery, Mire became the "type" star of the long-period " ira variables ".
	www.musicians-resource.com /site/44197-sealy-mira-loma.html (576 words)

	Mira, Omicron Ceti
		Johann Hevelius observed it from 1659 to 1682, inserted it in his monumental work, Prodomus Astronomiae, and christened it "Mira", "the Wonderful", in his Historiola Mirae Stellae of 1662.
		The period of Mira was first determined more acurately by Ismail Bouillaud of Paris to be 333 days, only about 1 day deviating from the modern value, no wonder because this period is subject to small irregular variations.
		Because of the form of its light curve, Mira is roughly visible to the naked eye (i.e., brighter than about 6th mag) for 1.5 months before and 2.5 to 3 months after its maximum.
	seds.lpl.arizona.edu /~spider/spider/Vars/mira.html (668 words)

	Early Variable Star Discoverers
		Discovered Nova 1783 Sagittae, also named WY Sagittae (WY Sge)
		Ismail Bouillaud (Bullialdus; Sep 28, 1605 - Nov 25, 1694)
		Observed Mira (Omicron Ceti) and found its period to be about 333 days.
	www.seds.org /%7Espider/spider/Vars/Add/var-dis.html (728 words)

	JBC -- Table of Contents (Aug 29 2003, 278, (35))
		Claire Tiraby, Geneviève Tavernier, Corinne Lefort, Dominique Larrouy, Frédéric Bouillaud, Daniel Ricquier, and Dominique Langin
		Thamir M. Ismail, C. Anthony Hart, and Alexander G. McLennan
		Jinhe Li, Gregory J. Fici, Chai-An Mao, Richard L. Myers, Rongqing Shuang, Gregory P. Donoho, Adele M. Pauley, Carol S. Himes, Wenning Qin, Ismail Kola, Kalpana M. Merchant, and Jeffrey S. Nye
	www.jbc.org /content/vol278/issue35/index.shtml (4001 words)

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