Analysis of light curve of LP Camelopardalis

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F16%3A00090010" target="_blank" >RIV/00216224:14310/16:00090010 - isvavai.cz</a>

Result on the web

<a href="http://www.konkoly.hu/Mitteilungen/105.html" target="_blank" >http://www.konkoly.hu/Mitteilungen/105.html</a>

DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Analysis of light curve of LP Camelopardalis

Original language description

We present photometric analysis of the RRab type pulsating star LP Cam. The star was observed at Brno Observatory and Planetarium during nine nights. Measurements were calibrated to the Johnson photometric system. Four captured and thirteen previously published maxima timings allowed us to refine the pulsation period and the zero epoch. The light curve was Fourier decomposed to estimate physical parameters using empirical relations. Our results suggest that LP Cam is a common RR Lyrae star with high, almost solar metallicity.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/LH14300" target="_blank" >LH14300: Investigations of curious variable stars</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Publication year

2016

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Communications from the Konkoly Observatory 105

ISBN

9638361565

ISSN

0238-2091

e-ISSN

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Number of pages

2

Pages from-to

213-214

Publisher name

NestPress Kft.

Place of publication

Budapest

Event location

Visegrád

Event date

Jan 1, 2015

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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