Light curves and period changes of type II cepheids in the globular clusters M3 and M5

Katie Rabidoux; Horace A. Smith; Barton J. Pritzl; Wayne Osborn; Charles Kuehn; Jill Randall; R. Lustig; K. Wells; Lisa Taylor; Nathan De Lee; K. Kinemuchi; Aaron Lacluyzé; D. Hartley; C. Greenwood; M. Ingber; M. Ireland; E. Pellegrini; Mary Anderson; Gene Purdum; J. Lacy; M. Curtis; Jason Smolinski; Stephen Danford

doi:10.1088/0004-6256/139/6/2300

Light curves and period changes of type II cepheids in the globular clusters M3 and M5

Katie Rabidoux, Horace A. Smith, Barton J. Pritzl, Wayne Osborn, Charles Kuehn, Jill Randall, R. Lustig, K. Wells, Lisa Taylor, Nathan De Lee, K. Kinemuchi, Aaron Lacluyzé, D. Hartley, C. Greenwood, M. Ingber, M. Ireland, E. Pellegrini, Mary Anderson, Gene Purdum, J. LacyM. Curtis, Jason Smolinski, Stephen Danford

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

12 Citations (Scopus)

Abstract

Light curves in the B, V, and Ic passbands have been obtained for the type II Cepheids V154 in M3 and V42 and V84 in M5. Alternating cycle behavior, similar to that seen among RV Tauri variables, is confirmed for V84. Old and new observations, spanning more than a century, show that V154 has increased in period while V42 has decreased in period. V84, on the other hand, has shown large, erratic changes in period that do not appear to reflect the long-term evolution of V84 through the Hertzsprung-Russel diagram.

Original language	English
Pages (from-to)	2300-2307
Number of pages	8
Journal	The Astronomical Journal
Volume	139
Issue number	6
DOIs	https://doi.org/10.1088/0004-6256/139/6/2300
Publication status	Published - 2010
Externally published	Yes

Keywords

Globular clusters: individual (NGC 5272, NGC 5904)
Stars: variables: Cepheids

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10.1088/0004-6256/139/6/2300

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Rabidoux, K., Smith, H. A., Pritzl, B. J., Osborn, W., Kuehn, C., Randall, J., Lustig, R., Wells, K., Taylor, L., De Lee, N., Kinemuchi, K., Lacluyzé, A., Hartley, D., Greenwood, C., Ingber, M., Ireland, M., Pellegrini, E., Anderson, M., Purdum, G., ... Danford, S. (2010). Light curves and period changes of type II cepheids in the globular clusters M3 and M5. The Astronomical Journal, 139(6), 2300-2307. https://doi.org/10.1088/0004-6256/139/6/2300

@article{736135d5795248ca98061907002c66e1,

title = "Light curves and period changes of type II cepheids in the globular clusters M3 and M5",

abstract = "Light curves in the B, V, and Ic passbands have been obtained for the type II Cepheids V154 in M3 and V42 and V84 in M5. Alternating cycle behavior, similar to that seen among RV Tauri variables, is confirmed for V84. Old and new observations, spanning more than a century, show that V154 has increased in period while V42 has decreased in period. V84, on the other hand, has shown large, erratic changes in period that do not appear to reflect the long-term evolution of V84 through the Hertzsprung-Russel diagram.",

keywords = "Globular clusters: individual (NGC 5272, NGC 5904), Stars: variables: Cepheids",

author = "Katie Rabidoux and Smith, {Horace A.} and Pritzl, {Barton J.} and Wayne Osborn and Charles Kuehn and Jill Randall and R. Lustig and K. Wells and Lisa Taylor and {De Lee}, Nathan and K. Kinemuchi and Aaron Lacluyz{\'e} and D. Hartley and C. Greenwood and M. Ingber and M. Ireland and E. Pellegrini and Mary Anderson and Gene Purdum and J. Lacy and M. Curtis and Jason Smolinski and Stephen Danford",

year = "2010",

doi = "10.1088/0004-6256/139/6/2300",

language = "English",

volume = "139",

pages = "2300--2307",

journal = "The Astronomical Journal",

issn = "0004-6256",

publisher = "Institute of Physics",

number = "6",

}

Rabidoux, K, Smith, HA, Pritzl, BJ, Osborn, W, Kuehn, C, Randall, J, Lustig, R, Wells, K, Taylor, L, De Lee, N, Kinemuchi, K, Lacluyzé, A, Hartley, D, Greenwood, C, Ingber, M, Ireland, M, Pellegrini, E, Anderson, M, Purdum, G, Lacy, J, Curtis, M, Smolinski, J & Danford, S 2010, 'Light curves and period changes of type II cepheids in the globular clusters M3 and M5', The Astronomical Journal, vol. 139, no. 6, pp. 2300-2307. https://doi.org/10.1088/0004-6256/139/6/2300

TY - JOUR

T1 - Light curves and period changes of type II cepheids in the globular clusters M3 and M5

AU - Rabidoux, Katie

AU - Smith, Horace A.

AU - Pritzl, Barton J.

AU - Osborn, Wayne

AU - Kuehn, Charles

AU - Randall, Jill

AU - Lustig, R.

AU - Wells, K.

AU - Taylor, Lisa

AU - De Lee, Nathan

AU - Kinemuchi, K.

AU - Lacluyzé, Aaron

AU - Hartley, D.

AU - Greenwood, C.

AU - Ingber, M.

AU - Ireland, M.

AU - Pellegrini, E.

AU - Anderson, Mary

AU - Purdum, Gene

AU - Lacy, J.

AU - Curtis, M.

AU - Smolinski, Jason

AU - Danford, Stephen

PY - 2010

Y1 - 2010

N2 - Light curves in the B, V, and Ic passbands have been obtained for the type II Cepheids V154 in M3 and V42 and V84 in M5. Alternating cycle behavior, similar to that seen among RV Tauri variables, is confirmed for V84. Old and new observations, spanning more than a century, show that V154 has increased in period while V42 has decreased in period. V84, on the other hand, has shown large, erratic changes in period that do not appear to reflect the long-term evolution of V84 through the Hertzsprung-Russel diagram.

AB - Light curves in the B, V, and Ic passbands have been obtained for the type II Cepheids V154 in M3 and V42 and V84 in M5. Alternating cycle behavior, similar to that seen among RV Tauri variables, is confirmed for V84. Old and new observations, spanning more than a century, show that V154 has increased in period while V42 has decreased in period. V84, on the other hand, has shown large, erratic changes in period that do not appear to reflect the long-term evolution of V84 through the Hertzsprung-Russel diagram.

KW - Globular clusters: individual (NGC 5272, NGC 5904)

KW - Stars: variables: Cepheids

U2 - 10.1088/0004-6256/139/6/2300

DO - 10.1088/0004-6256/139/6/2300

M3 - Article

SN - 0004-6256

VL - 139

SP - 2300

EP - 2307

JO - The Astronomical Journal

JF - The Astronomical Journal

IS - 6

ER -

Light curves and period changes of type II cepheids in the globular clusters M3 and M5

Abstract

Keywords

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