CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

Resultado de la investigación

Resumen

CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.
Idioma originalEnglish
Páginas (desde-hasta)161-162
PublicaciónThe Minor Planet Bulletin
Volumen35
EstadoPublished - 1 oct 2008

Huella dactilar

asteroid
observatory

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title = "CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory",
abstract = "CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.",
author = "Sada, {Pedro V.}",
year = "2008",
month = "10",
day = "1",
language = "English",
volume = "35",
pages = "161--162",
journal = "The Minor Planet Bulletin",
issn = "1052-8091",

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TY - JOUR

T1 - CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

AU - Sada, Pedro V.

PY - 2008/10/1

Y1 - 2008/10/1

N2 - CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.

AB - CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.

M3 - Article

VL - 35

SP - 161

EP - 162

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -