Lightcurve Analysis of 1084 Tamariwa

Research output: Contribution to journalArticle

Abstract

Photometric observations of 1084 Tamariwa were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 6.1949 ± 0.0002 h and amplitude of ~0.32 mag.
Original languageEnglish
Pages (from-to)50
JournalThe Minor Planet Bulletin
Volume35
Publication statusPublished - 1 Jun 2008

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title = "Lightcurve Analysis of 1084 Tamariwa",
abstract = "Photometric observations of 1084 Tamariwa were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 6.1949 ± 0.0002 h and amplitude of ~0.32 mag.",
author = "Sada, {Pedro V.}",
year = "2008",
month = "6",
day = "1",
language = "English",
volume = "35",
pages = "50",
journal = "The Minor Planet Bulletin",
issn = "1052-8091",

}

Lightcurve Analysis of 1084 Tamariwa. / Sada, Pedro V.

In: The Minor Planet Bulletin, Vol. 35, 01.06.2008, p. 50.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Lightcurve Analysis of 1084 Tamariwa

AU - Sada, Pedro V.

PY - 2008/6/1

Y1 - 2008/6/1

N2 - Photometric observations of 1084 Tamariwa were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 6.1949 ± 0.0002 h and amplitude of ~0.32 mag.

AB - Photometric observations of 1084 Tamariwa were made during August and September of 2007. Analysis of the data yields a synodic rotational period of 6.1949 ± 0.0002 h and amplitude of ~0.32 mag.

M3 - Article

VL - 35

SP - 50

JO - The Minor Planet Bulletin

JF - The Minor Planet Bulletin

SN - 1052-8091

ER -