Abundances and Kinematics of OB Stars in the Leading Arm of the Magellanic System

Zhang L.; Moni Bidin C.; Casetti-Dinescu D. I.; Mendez R. A.; Girard T. M.; Korchagin V. I.; Vieira K.; van Altena W. F.; Zhao G.

Vol. 50 (2018), Contributions

Vol. 50 (2018)

Contributions

Abundances and Kinematics of OB Stars in the Leading Arm of the Magellanic System

Zhang L.⁺⁻
Moni Bidin C.⁺⁻
Casetti-Dinescu D. I.⁺⁻
Mendez R. A.⁺⁻
Girard T. M.⁺⁻
Korchagin V. I.⁺⁻
Vieira K.⁺⁻
van Altena W. F.⁺⁻
Zhao G.⁺⁻

Zhang L.

Key Lab for Optical Astronomy, National Astronomical Observatories, CAS, 20A Datun Road, Chaoyang District, 100012 Beijing, China

Moni Bidin C.

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Casetti-Dinescu D. I.

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Mendez R. A.

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Girard T. M.

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Korchagin V. I.

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Vieira K.

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van Altena W. F.

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Zhao G.

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Keywords

Magellanic Clouds
stars: abundances
stars: early-type

How to Cite

Abundances and Kinematics of OB Stars in the Leading Arm of the Magellanic System. (2018). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 50, 68-68. https://astronomia.unam.mx/journals/rmxac/article/view/2018rmxac..50...68z

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Abstract

We determined seven element abundances (He, C, N, O, Mg, Si, and S) and kinematics for eight O-/B- type stars which is selected from 42 candidates (Casetti-Dinescu et al. 2014) of membership in the Leading Arm (LA) of the Magellanic System. The high resolution spectra were taken with the MIKE instrument on the Magellan 6.5m Clay telescope.

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Abundances and Kinematics of OB Stars in the Leading Arm of the Magellanic System

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