Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-29T17:39:29.977Z Has data issue: false hasContentIssue false
  • English
  • Français

The Nature of the Triangulum-Andromeda Stellar Structures

Published online by Cambridge University Press:  30 October 2019

J. V. Sales Silva ,
H. Perottoni ,
K. Cunha ,
H. J. Rocha-Pinto ,
D. Souto  and
F. Almeida-Fernandes
J. V. Sales Silva
Affiliation:
Observatório Nacional/MCTIC Rua Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil emails: [email protected]; [email protected]; [email protected]
H. Perottoni
Affiliation:
Observatório do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antônio 43, 20080-090, Rio de Janeiro, Brazil, email: [email protected]
K. Cunha
Affiliation:
Observatório Nacional/MCTIC Rua Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil emails: [email protected]; [email protected]; [email protected] University of Arizona, Tucson, AZ 85719, USA
H. J. Rocha-Pinto
Affiliation:
Observatório do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antônio 43, 20080-090, Rio de Janeiro, Brazil, email: [email protected]
D. Souto
Affiliation:
Observatório Nacional/MCTIC Rua Gen. José Cristino, 77, 20921-400, Rio de Janeiro, Brazil emails: [email protected]; [email protected]; [email protected]
F. Almeida-Fernandes
Affiliation:
Observatório do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antônio 43, 20080-090, Rio de Janeiro, Brazil, email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The outer stellar halo is home to a number of substructures that are remnants of former interactions of the Galaxy with its dwarf satellites. Triangulum-Andromeda (TriAnd) is one of these halo substructures, found as a debris cloud by Rocha-Pinto et al., (2004) using 2MASS M giants. Would be these structures related to dwarf galaxies or to the galactic disk? To uncover the nature of these stars we performed a high-resolution spectroscopic study (R = 40,000) along with a kinematic analysis using Gaia data. We determined the atmospheric parameters and chemical abundances of Ca and Mg for the 13 TriAnd candidate stars along with their respective orbits. Our results indicate that the TriAnd stars analyzed have a galactic nature but that these stars are not from the local thin disk.

Keywords

Galaxy: structureGalaxy: outer diskstars: chemical abundancesstars: kinematic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 122 - 124
Copyright
© International Astronomical Union 2019 

References

Bensby, T., Feltzing, S., & Oey, M. S. 2014, A&A, 562, A71 Google Scholar
Bergemann, M., Sesar, B., Cohen, J. G., et al . 2018, Nature, 555, 334 CrossRefGoogle Scholar
Chene, A.-N., Padzer, J., Barrick, G., et al . 2014, PROCSPIE, 9151, 915147 Google Scholar
Chou, M.-Y., Majewski, S. R., Cunha, K., et al . 2011, Ap. Lett., 731, L30 CrossRefGoogle Scholar
Geisler, D., Smith, V. V., Wallerstein, G., Gonzalez, G., & Charbonnel, C. 2005, AJ, 129, 1428 CrossRefGoogle Scholar
Gómez, F. A., Minchev, I., O’Shea, B. W., et al . 2013, MNRAS, 429, 159 CrossRefGoogle Scholar
Gustafsson, B., Edvardsson, B., Eriksson, K., et al . 2008, A&A, 486, 951 Google Scholar
Hayes, C. R., Majewski, S. R., Hasselquist, S., et al . 2018, Ap. Lett., 859, L8 Google Scholar
Koch, A., Grebel, E. K., Gilmore, G. F., et al . 2008, AJ, 135, 1580 CrossRefGoogle Scholar
Letarte, B. 2007, Ph.D. Thesis,Google Scholar
Majewski, S. R., Schiavon, R. P., Frinchaboy, P. M., et al . 2017, AJ, 154, 94 CrossRefGoogle Scholar
Martin, N. F., Ibata, R. A., Rich, R. M., et al . 2014, ApJ, 787, 19 CrossRefGoogle Scholar
Martioli, E., Teeple, D., Manset, N., et al . 2012, PROCSPIE, 8451, 84512B Google Scholar
Monaco, L., Bellazzini, M., Bonifacio, P., et al . 2005, A&A, 441, 141 Google Scholar
Perottoni, H. D., Rocha-Pinto, H. J., Girardi, L., et al . 2018, MNRAS, 473, 1461 CrossRefGoogle Scholar
Rocha-Pinto, H. J., Majewski, S. R., Skrutskie, M. F., Crane, J. D., & Patterson, R. J. 2004, ApJ, 615, 732 CrossRefGoogle Scholar
Sbordone, L., Bonifacio, P., Buonanno, R., et al . 2007, A&A, 465, 815 Google Scholar
Shetrone, M., Venn, K. A., Tolstoy, E., et al . 2003, AJ, 125, 684 CrossRefGoogle Scholar
Sneden, C. A. 1973, Ph.D. Thesis, https://ui.adsabs.harvard.edu/abs/1973PhDT…….180S/abstractGoogle Scholar
Tollestrup, E. V., Pazder, J., Barrick, G., et al . 2012, PROCSPIE, 8446, 84462A Google Scholar
Yong, D., Carney, B. W., & Friel, E. D. 2012, AJ, 144, 95 CrossRefGoogle Scholar