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

^*Bu çalışma için yazışmadan sorumlu yazar

Araştırma sonucu: ???type-name??? › Makale › bilirkişi

2 Atıf (Scopus)

Özet

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.

Orijinal dil	İngilizce
Sayfa (başlangıç-bitiş)	504-513
Sayfa sayısı	10
Dergi	New Astronomy
Hacim	17
Basın numarası	5
DOI'lar	https://doi.org/10.1016/j.newast.2011.11.010
Yayın durumu	Yayınlandı - Tem 2012
Harici olarak yayınlandı	Evet

Finansman

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.

Finansörler	Finansör numarası
TÜBİTAK	TBAG-108T475
Çukurova Üniversitesi	TBMYO2010BAP4, BAP-2010/40
Atatürk Üniversitesi

Belgeye Erişim

10.1016/j.newast.2011.11.010

Diğer Dosyalar ve Linkler

Link to publication in Scopus

Alıntı Yap

@article{103bccc19368437294f41959e2dcd202,

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",

issn = "1384-1076",

publisher = "Elsevier B.V.",

number = "5",

}

TY - JOUR

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

Özet

Finansman

Belgeye Erişim

Diğer Dosyalar ve Linkler

Parmak izi

Alıntı Yap