New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm

D. Majaess; D. Turner; C. Moni Bidin; F. Mauro; D. Geisler; W. Gieren; A.-N. Chené; D. Minniti; R.K. Saito; D. Minniti; D. Minniti; A.-N. Chené; J. Borissova; R. Kurtev; P.W. Lucas; I. Dékny

doi:10.1088/2041-8205/741/2/L27

New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm

D. Majaess, D. Turner, C. Moni Bidin, F. Mauro, D. Geisler, W. Gieren, A.-N. Chené, D. Minniti, R.K. Saito, D. Minniti, D. Minniti, A.-N. Chené, J. Borissova, R. Kurtev, P.W. Lucas, I. Dékny

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Abstract

The putative association between the 10. 8 classical Cepheid TW Nor and the open cluster Lyngå 6 has generated considerable debate in the literature.NewJHK photometry in tandem with existing radial velocities for Lyngå 6 stars implies cluster membership for TWNor and establishes the variable as a high-weight calibrator for classical Cepheid relations. Fundamental mean parameters determined forLyngå 6 are: d = 1.91±0.10 kpc,E(JH) = 0.38±0.02, and log τ= 7.9 ± 0.1. The Benedict et al./Turner Galactic VIc Wesenheit function was revised using TW Nor's new parameters:W = (3.37±0.08) log P 2.48±0.08. TW Nor/Lyngå 6 lie beyond the Sagittarius-Carina spiral arm and occupy the Centaurus arm, along with innumerable young Cepheids and clusters (e.g., VW Cen and VVV CL070).

Original language	English
Article number	L27
Number of pages	4
Journal	Astrophysical Journal Letters
Volume	741
Issue number	2
DOIs	https://doi.org/10.1088/2041-8205/741/2/L27
Publication status	Published - 2011

Keywords

dust, extinction
Hertzsprung-Russell and C-M diagrams
infrared: stars
open clusters and associations: individual: (Lynga 6)
stars: distances
stars: variables: Cepheids

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10.1088/2041-8205/741/2/L27

906046
‘In these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.’ Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical Society
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Majaess, D., Turner, D., Moni Bidin, C., Mauro, F., Geisler, D., Gieren, W., Chené, A.-N., Minniti, D., Saito, R. K., Minniti, D., Minniti, D., Chené, A.-N., Borissova, J., Kurtev, R., Lucas, P. W., & Dékny, I. (2011). New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm. Astrophysical Journal Letters, 741(2), Article L27. https://doi.org/10.1088/2041-8205/741/2/L27

@article{df0d69d0075e41f79d447bef35893500,

title = "New evidence supporting membership for TW nor in Lyng{\aa} 6 and the centaurus spiral arm",

abstract = "The putative association between the 10. 8 classical Cepheid TW Nor and the open cluster Lyng{\aa} 6 has generated considerable debate in the literature.NewJHK photometry in tandem with existing radial velocities for Lyng{\aa} 6 stars implies cluster membership for TWNor and establishes the variable as a high-weight calibrator for classical Cepheid relations. Fundamental mean parameters determined forLyng{\aa} 6 are: d = 1.91±0.10 kpc,E(JH) = 0.38±0.02, and log τ= 7.9 ± 0.1. The Benedict et al./Turner Galactic VIc Wesenheit function was revised using TW Nor's new parameters:W = (3.37±0.08) log P 2.48±0.08. TW Nor/Lyng{\aa} 6 lie beyond the Sagittarius-Carina spiral arm and occupy the Centaurus arm, along with innumerable young Cepheids and clusters (e.g., VW Cen and VVV CL070).",

keywords = "dust, extinction, Hertzsprung-Russell and C-M diagrams, infrared: stars, open clusters and associations: individual: (Lynga 6), stars: distances, stars: variables: Cepheids",

author = "D. Majaess and D. Turner and \{Moni Bidin\}, C. and F. Mauro and D. Geisler and W. Gieren and A.-N. Chen{\'e} and D. Minniti and R.K. Saito and D. Minniti and D. Minniti and A.-N. Chen{\'e} and J. Borissova and R. Kurtev and P.W. Lucas and I. D{\'e}kny",

note = "{\textquoteleft}In these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.{\textquoteright} Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical Society",

year = "2011",

doi = "10.1088/2041-8205/741/2/L27",

language = "English",

volume = "741",

journal = "Astrophysical Journal Letters",

issn = "2041-8213",

publisher = "American Astronomical Society",

number = "2",

}

Majaess, D, Turner, D, Moni Bidin, C, Mauro, F, Geisler, D, Gieren, W, Chené, A-N, Minniti, D, Saito, RK, Minniti, D, Minniti, D, Chené, A-N, Borissova, J, Kurtev, R, Lucas, PW & Dékny, I 2011, 'New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm', Astrophysical Journal Letters, vol. 741, no. 2, L27. https://doi.org/10.1088/2041-8205/741/2/L27

TY - JOUR

T1 - New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm

AU - Majaess, D.

AU - Turner, D.

AU - Moni Bidin, C.

AU - Mauro, F.

AU - Geisler, D.

AU - Gieren, W.

AU - Chené, A.-N.

AU - Minniti, D.

AU - Saito, R.K.

AU - Minniti, D.

AU - Chené, A.-N.

AU - Borissova, J.

AU - Kurtev, R.

AU - Lucas, P.W.

AU - Dékny, I.

N1 - ‘In these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.’ Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical Society

PY - 2011

Y1 - 2011

N2 - The putative association between the 10. 8 classical Cepheid TW Nor and the open cluster Lyngå 6 has generated considerable debate in the literature.NewJHK photometry in tandem with existing radial velocities for Lyngå 6 stars implies cluster membership for TWNor and establishes the variable as a high-weight calibrator for classical Cepheid relations. Fundamental mean parameters determined forLyngå 6 are: d = 1.91±0.10 kpc,E(JH) = 0.38±0.02, and log τ= 7.9 ± 0.1. The Benedict et al./Turner Galactic VIc Wesenheit function was revised using TW Nor's new parameters:W = (3.37±0.08) log P 2.48±0.08. TW Nor/Lyngå 6 lie beyond the Sagittarius-Carina spiral arm and occupy the Centaurus arm, along with innumerable young Cepheids and clusters (e.g., VW Cen and VVV CL070).

AB - The putative association between the 10. 8 classical Cepheid TW Nor and the open cluster Lyngå 6 has generated considerable debate in the literature.NewJHK photometry in tandem with existing radial velocities for Lyngå 6 stars implies cluster membership for TWNor and establishes the variable as a high-weight calibrator for classical Cepheid relations. Fundamental mean parameters determined forLyngå 6 are: d = 1.91±0.10 kpc,E(JH) = 0.38±0.02, and log τ= 7.9 ± 0.1. The Benedict et al./Turner Galactic VIc Wesenheit function was revised using TW Nor's new parameters:W = (3.37±0.08) log P 2.48±0.08. TW Nor/Lyngå 6 lie beyond the Sagittarius-Carina spiral arm and occupy the Centaurus arm, along with innumerable young Cepheids and clusters (e.g., VW Cen and VVV CL070).

KW - dust, extinction

KW - Hertzsprung-Russell and C-M diagrams

KW - infrared: stars

KW - open clusters and associations: individual: (Lynga 6)

KW - stars: distances

KW - stars: variables: Cepheids

UR - https://www.scopus.com/pages/publications/80655149264

U2 - 10.1088/2041-8205/741/2/L27

DO - 10.1088/2041-8205/741/2/L27

M3 - Article

AN - SCOPUS:80655149264

SN - 2041-8213

VL - 741

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L27

ER -

New evidence supporting membership for TW nor in Lyngå 6 and the centaurus spiral arm

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Keywords

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