Kinematic imprints from the bar and spiral structures in the galatic disk

F. Figueras; Teresa Antoja Castelltort; O. Valenzuela; M. Romero-Gómez; B. Pichardo; E. Moreno

Kinematic imprints from the bar and spiral structures in the galatic disk

F. Figueras, Teresa Antoja Castelltort, O. Valenzuela, M. Romero-Gómez, B. Pichardo, E. Moreno

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

Abstract

At 140 years of the discovery of the moving groups, these stellar streams are emerging as powerful tools to constrain the models for the spiral arms and the Galactic bar in the Gaia era. From the kinematic-age-metallicity analysis in the solar neighbourhood it is now well established that some of these kinematic structures have a dynamical origin, different from the classical cluster disruption hypothesis. Test particle simulations allow us to definitively establish that these local structures can be created by the dynamical resonances

Original language	English
Title of host publication	SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290
Subtitle of host publication	Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Editors	G. Alecian, K. Belkacem, R. Samadi, D. Valls-Gabaud
Pages	287-290
Number of pages	4
Publication status	Published - Dec-2011

Keywords

Galaxy: kinematics and dynamics
solar neighbourhood
spiral structure
Galactic bar

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Figueras, F., Antoja Castelltort, T., Valenzuela, O., Romero-Gómez, M., Pichardo, B., & Moreno, E. (2011). Kinematic imprints from the bar and spiral structures in the galatic disk. In G. Alecian, K. Belkacem, R. Samadi, & D. Valls-Gabaud (Eds.), SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics (pp. 287-290) http://adsabs.harvard.edu/abs/2011sf2a.conf..287F

Figueras, F. ; Antoja Castelltort, Teresa ; Valenzuela, O. et al. / Kinematic imprints from the bar and spiral structures in the galatic disk. SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. editor / G. Alecian ; K. Belkacem ; R. Samadi ; D. Valls-Gabaud. 2011. pp. 287-290

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title = "Kinematic imprints from the bar and spiral structures in the galatic disk",

abstract = "At 140 years of the discovery of the moving groups, these stellar streams are emerging as powerful tools to constrain the models for the spiral arms and the Galactic bar in the Gaia era. From the kinematic-age-metallicity analysis in the solar neighbourhood it is now well established that some of these kinematic structures have a dynamical origin, different from the classical cluster disruption hypothesis. Test particle simulations allow us to definitively establish that these local structures can be created by the dynamical resonances",

keywords = "Galaxy: kinematics and dynamics, solar neighbourhood, spiral structure, Galactic bar",

author = "F. Figueras and {Antoja Castelltort}, Teresa and O. Valenzuela and M. Romero-G{\'o}mez and B. Pichardo and E. Moreno",

note = "M1 - Conference Proceedings",

year = "2011",

month = dec,

language = "English",

pages = "287--290",

editor = "G. Alecian and K. Belkacem and R. Samadi and D. Valls-Gabaud",

booktitle = "SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290",

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Figueras, F, Antoja Castelltort, T, Valenzuela, O, Romero-Gómez, M, Pichardo, B & Moreno, E 2011, Kinematic imprints from the bar and spiral structures in the galatic disk. in G Alecian, K Belkacem, R Samadi & D Valls-Gabaud (eds), SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. pp. 287-290. <http://adsabs.harvard.edu/abs/2011sf2a.conf..287F>

Kinematic imprints from the bar and spiral structures in the galatic disk. / Figueras, F.; Antoja Castelltort, Teresa; Valenzuela, O. et al.
SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. ed. / G. Alecian; K. Belkacem; R. Samadi; D. Valls-Gabaud. 2011. p. 287-290.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

TY - GEN

T1 - Kinematic imprints from the bar and spiral structures in the galatic disk

AU - Figueras, F.

AU - Antoja Castelltort, Teresa

AU - Valenzuela, O.

AU - Romero-Gómez, M.

AU - Pichardo, B.

AU - Moreno, E.

N1 - M1 - Conference Proceedings

PY - 2011/12

Y1 - 2011/12

N2 - At 140 years of the discovery of the moving groups, these stellar streams are emerging as powerful tools to constrain the models for the spiral arms and the Galactic bar in the Gaia era. From the kinematic-age-metallicity analysis in the solar neighbourhood it is now well established that some of these kinematic structures have a dynamical origin, different from the classical cluster disruption hypothesis. Test particle simulations allow us to definitively establish that these local structures can be created by the dynamical resonances

AB - At 140 years of the discovery of the moving groups, these stellar streams are emerging as powerful tools to constrain the models for the spiral arms and the Galactic bar in the Gaia era. From the kinematic-age-metallicity analysis in the solar neighbourhood it is now well established that some of these kinematic structures have a dynamical origin, different from the classical cluster disruption hypothesis. Test particle simulations allow us to definitively establish that these local structures can be created by the dynamical resonances

KW - Galaxy: kinematics and dynamics

KW - solar neighbourhood

KW - spiral structure

KW - Galactic bar

M3 - Conference contribution

SP - 287

EP - 290

BT - SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290

A2 - Alecian, G.

A2 - Belkacem, K.

A2 - Samadi, R.

A2 - Valls-Gabaud, D.

ER -

Figueras F, Antoja Castelltort T, Valenzuela O, Romero-Gómez M, Pichardo B, Moreno E. Kinematic imprints from the bar and spiral structures in the galatic disk. In Alecian G, Belkacem K, Samadi R, Valls-Gabaud D, editors, SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem, R. Samadi and D. Valls-Gabaud, pp.287-290: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. 2011. p. 287-290

Kinematic imprints from the bar and spiral structures in the galatic disk

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Keywords

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