Two New Eclipsing Binary Systems: GSC 1393-1461 and GSC 2449-0654, and One New Flare Star: GSC 5604-0255

Research output: Contribution to journalArticle

Abstract

We introduce three new variable stars discovered during asteroid photometry. This includes two new eclipsing binary stars, GSC 1393-1461 (P = 0.311145d) and GSC 2449-0654 (P = 0.343802d), and one new flare star: GSC 5604-0255, which had a 35% ± 2% intensity increase with a decay half-life of 20 ± 1 minutes. This paper presents light curves along with basic models and analysis of the data.
Original languageEnglish
Pages (from-to)52
JournalThe Journal of the American Association of Variable Star Observers
Volume38
Publication statusPublished - 1 Jun 2010
Externally publishedYes

Fingerprint

eclipsing binary stars
flare stars
variable stars
half life
decay

Cite this

@article{bc2f745bb0774bbea1d0d5119fda9776,
title = "Two New Eclipsing Binary Systems: GSC 1393-1461 and GSC 2449-0654, and One New Flare Star: GSC 5604-0255",
abstract = "We introduce three new variable stars discovered during asteroid photometry. This includes two new eclipsing binary stars, GSC 1393-1461 (P = 0.311145d) and GSC 2449-0654 (P = 0.343802d), and one new flare star: GSC 5604-0255, which had a 35{\%} ± 2{\%} intensity increase with a decay half-life of 20 ± 1 minutes. This paper presents light curves along with basic models and analysis of the data.",
author = "Sada, {P. V.}",
year = "2010",
month = "6",
day = "1",
language = "English",
volume = "38",
pages = "52",
journal = "The Journal of the American Association of Variable Star Observers",

}

TY - JOUR

T1 - Two New Eclipsing Binary Systems: GSC 1393-1461 and GSC 2449-0654, and One New Flare Star: GSC 5604-0255

AU - Sada, P. V.

PY - 2010/6/1

Y1 - 2010/6/1

N2 - We introduce three new variable stars discovered during asteroid photometry. This includes two new eclipsing binary stars, GSC 1393-1461 (P = 0.311145d) and GSC 2449-0654 (P = 0.343802d), and one new flare star: GSC 5604-0255, which had a 35% ± 2% intensity increase with a decay half-life of 20 ± 1 minutes. This paper presents light curves along with basic models and analysis of the data.

AB - We introduce three new variable stars discovered during asteroid photometry. This includes two new eclipsing binary stars, GSC 1393-1461 (P = 0.311145d) and GSC 2449-0654 (P = 0.343802d), and one new flare star: GSC 5604-0255, which had a 35% ± 2% intensity increase with a decay half-life of 20 ± 1 minutes. This paper presents light curves along with basic models and analysis of the data.

M3 - Article

VL - 38

SP - 52

JO - The Journal of the American Association of Variable Star Observers

JF - The Journal of the American Association of Variable Star Observers

ER -