Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017

M. E. Contreras; L. Olguín; P. Loera-González; J. C. Saucedo; S. Estrada-Dorado; A. López-López; C. A. Medina; J. C. Ramírez; R. Núñez-López; Pedro V. Sada

Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017

M. E. Contreras, L. Olguín, P. Loera-González, J. C. Saucedo, S. Estrada-Dorado, A. López-López, C. A. Medina, J. C. Ramírez, R. Núñez-López, Pedro V. Sada

Departamento de Física y Matemáticas

Resultado de la investigación › revisión exhaustiva

Resumen

We present photometric lightcurves and rotation period values for three asteroids, namely 4404 Enirac (2.9986 ± 0.0003 h), 5976 Kalatajean (4.5543 ± 0.0001 h) and 9671 Hemera (2.5323 ± 0.0005 h). Observations were carried out at the Carl Sagan Observatory (OCS) of the Universidad de Sonora. In the case of 9671 Hemera we have not found any clear evidence of binarity.

Idioma original	English
Páginas (desde-hasta)	233-234
Número de páginas	2
Publicación	The Minor Planet Bulletin
Volumen	46
Estado	Published - 1 jul 2019

Acceder al documento

http://adsabs.harvard.edu/abs/2019MPBu...46..233C

Huella Profundice en los temas de investigación de 'Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017'. En conjunto forman una huella única.

Citar esto

@article{570db5e03e5f4b818eb12c0492f8acd9,

title = "Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017",

abstract = "We present photometric lightcurves and rotation period values for three asteroids, namely 4404 Enirac (2.9986 ± 0.0003 h), 5976 Kalatajean (4.5543 ± 0.0001 h) and 9671 Hemera (2.5323 ± 0.0005 h). Observations were carried out at the Carl Sagan Observatory (OCS) of the Universidad de Sonora. In the case of 9671 Hemera we have not found any clear evidence of binarity.",

author = "Contreras, {M. E.} and L. Olgu{\'i}n and P. Loera-Gonz{\'a}lez and Saucedo, {J. C.} and S. Estrada-Dorado and A. L{\'o}pez-L{\'o}pez and Medina, {C. A.} and Ram{\'i}rez, {J. C.} and R. N{\'u}{\~n}ez-L{\'o}pez and Sada, {Pedro V.}",

year = "2019",

month = jul,

day = "1",

language = "English",

volume = "46",

pages = "233--234",

journal = "The Minor Planet Bulletin",

issn = "1052-8091",

}

Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017. / Contreras, M. E.; Olguín, L.; Loera-González, P.; Saucedo, J. C.; Estrada-Dorado, S.; López-López, A.; Medina, C. A.; Ramírez, J. C.; Núñez-López, R.; Sada, Pedro V.

En: The Minor Planet Bulletin, Vol. 46, 01.07.2019, p. 233-234.

Resultado de la investigación › revisión exhaustiva

TY - JOUR

T1 - Asteroid Photometry at the Carl Sagan Observatory of Universidad De Sonora During 2017

AU - Contreras, M. E.

AU - Olguín, L.

AU - Loera-González, P.

AU - Saucedo, J. C.

AU - Estrada-Dorado, S.

AU - López-López, A.

AU - Medina, C. A.

AU - Ramírez, J. C.

AU - Núñez-López, R.

AU - Sada, Pedro V.

PY - 2019/7/1

Y1 - 2019/7/1

N2 - We present photometric lightcurves and rotation period values for three asteroids, namely 4404 Enirac (2.9986 ± 0.0003 h), 5976 Kalatajean (4.5543 ± 0.0001 h) and 9671 Hemera (2.5323 ± 0.0005 h). Observations were carried out at the Carl Sagan Observatory (OCS) of the Universidad de Sonora. In the case of 9671 Hemera we have not found any clear evidence of binarity.

AB - We present photometric lightcurves and rotation period values for three asteroids, namely 4404 Enirac (2.9986 ± 0.0003 h), 5976 Kalatajean (4.5543 ± 0.0001 h) and 9671 Hemera (2.5323 ± 0.0005 h). Observations were carried out at the Carl Sagan Observatory (OCS) of the Universidad de Sonora. In the case of 9671 Hemera we have not found any clear evidence of binarity.

M3 - Article

VL - 46

SP - 233

EP - 234

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -