Long-term variations and periods of Mira stars from ROTSE-IIId

C. Yeşilyaprak; S. K. Yerli; B. B. Güsav; N. Aksaker; E. Dikiciolu; M. Helvaci; D. Oker; M. E. Aydin; B. Dinel; N. Uzun

doi:10.1016/j.newast.2011.11.010

Long-term variations and periods of Mira stars from ROTSE-IIId

C. Yeşilyaprak^*, S. K. Yerli, B. B. Güsav, N. Aksaker, E. Dikiciolu, M. Helvaci, D. Oker, M. E. Aydin, B. Dinel, N. Uzun

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TÜBTAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables, 17 periods are identified for the first time.

Original language	English
Pages (from-to)	504-513
Number of pages	10
Journal	New Astronomy
Volume	17
Issue number	5
DOIs	https://doi.org/10.1016/j.newast.2011.11.010
Publication status	Published - Jul 2012
Externally published	Yes

Funding

This study was supported by TÜBİTAK with the project TBAG-108T475 and also supported with Scientific Research Project of Atatürk University and Çukurova University with Grant No. BAP-2010/40 and TBMYO2010BAP4 , respectively.

Funders	Funder number
TÜBİTAK	TBAG-108T475
Çukurova Üniversitesi	TBMYO2010BAP4, BAP-2010/40
Atatürk Üniversitesi

Keywords

Methods: data analysis
Stars: late-type

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10.1016/j.newast.2011.11.010

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title = "Long-term variations and periods of Mira stars from ROTSE-IIId",

abstract = "We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at T{\"U}BTAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables, 17 periods are identified for the first time.",

keywords = "Methods: data analysis, Stars: late-type",

author = "C. Ye{\c s}ilyaprak and Yerli, {S. K.} and G{\"u}sav, {B. B.} and N. Aksaker and E. Dikiciolu and M. Helvaci and D. Oker and Aydin, {M. E.} and B. Dinel and N. Uzun",

year = "2012",

month = jul,

doi = "10.1016/j.newast.2011.11.010",

language = "English",

volume = "17",

pages = "504--513",

journal = "New Astronomy",

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T1 - Long-term variations and periods of Mira stars from ROTSE-IIId

AU - Yeşilyaprak, C.

AU - Yerli, S. K.

AU - Güsav, B. B.

AU - Aksaker, N.

AU - Dikiciolu, E.

AU - Helvaci, M.

AU - Oker, D.

AU - Aydin, M. E.

AU - Dinel, B.

AU - Uzun, N.

PY - 2012/7

Y1 - 2012/7

N2 - We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TÜBTAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables, 17 periods are identified for the first time.

AB - We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TÜBTAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables, 17 periods are identified for the first time.

KW - Methods: data analysis

KW - Stars: late-type

UR - http://www.scopus.com/inward/record.url?scp=84856266077&partnerID=8YFLogxK

U2 - 10.1016/j.newast.2011.11.010

DO - 10.1016/j.newast.2011.11.010

M3 - Article

AN - SCOPUS:84856266077

SN - 1384-1076

VL - 17

SP - 504

EP - 513

JO - New Astronomy

JF - New Astronomy

IS - 5

ER -

Long-term variations and periods of Mira stars from ROTSE-IIId

Abstract

Funding

Keywords

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