ORBi: Debehogne H. - Photoelectric light curves of minor planets 599 Luisa and 128 Nemesis during the 1976 opposition

Reference : Photoelectric light curves of minor planets 599 Luisa and 128 Nemesis during the 1976 op...


	Document type :	Scientific journals : Article
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/17732

Title :	Photoelectric light curves of minor planets 599 Luisa and 128 Nemesis during the 1976 opposition
Language :	English
Author, co-author :	Debehogne, H. [Observatoire Royal de Belgique, Brussels, Belgium]
	Surdej, Anna [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
	Surdej, Jean [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Publication date :	1977
Journal title :	Astronomy and Astrophysics. Supplement Series
Publisher :	EDP Sciences
Volume :	30
Pages :	375-379
Audience :	International
ISSN :	0365-0138
City :	Les Ulis
Country :	France
Keywords :	[en] ASTRONOMICAL PHOTOMETRY ; ELECTROPHOTOMETRY ; LIGHT CURVE ; ASTRONOMICAL COORDINATES ; PLANETARY ROTATION ; UBV SPECTRA ; ASTEROIDS
Abstract :	[en] Asteroids 599 Luisa and 128 Nemesis were observed photometrically at the European Southern Observatory during the 1976 opposition. The light curve of 599 Luisa shows two well-shaped minima and maxima together with a short-time-scale feature. The synodic period of rotation found for 599 Luisa 9 hr 33 min 58 (+ or -46) sec, and the maximum amplitude of the light curve is 0.18 mag. Minor planet 128 Nemesis could only be observed during one night and appears to be a slowly rotating asteroid.
Target :	Researchers ; Professionals
Permalink :	http://hdl.handle.net/2268/17732
Other URL :	http://esoads.eso.org/abs/1977A%26AS...30..375D
Mentions required by the publisher for OA :	A&AA ID. AAA020.098.046 The authors thank EDP Sciences for their deposit authorization

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