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APOGEE DR14/DR15 Abundances in the Inner Milky Way

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:43

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The bimodal [Mg/Fe] versus [Fe/H] bulge sequence as revealed by APOGEE DR14

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:38

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H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:29

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Globular cluster candidates in the Galactic bulge: Gaia and VVV view of the latest discoveries

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:26

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The origin of stellar populations in the Galactic bulge from chemical abundances

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:18

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The chemistry of stars in the bar of the Milky Way

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:16

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Using classical Cepheids to study the far side of the Milky Way disk. I. Spectroscopic classification and the metallicity gradient

Enviado por Valeria.salas en Jue, 01/04/2024 - 11:14

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Cool stars in the Galactic center as seen by APOGEE. M giants, AGB stars, and supergiant stars and candidates

Enviado por Valeria.salas en Jue, 01/04/2024 - 10:57

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How many components? Quantifying the complexity of the metallicity distribution in the Milky Way bulge with APOGEE

Enviado por Valeria.salas en Jue, 01/04/2024 - 10:55

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The diffuse interstellar band around 8620 Å. I. Methods and application to the GIBS data set

Enviado por Valeria.salas en Jue, 01/04/2024 - 10:49

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Leer más sobre The diffuse interstellar band around 8620 Å. I. Methods and application to the GIBS data set

APOGEE DR14/DR15 Abundances in the Inner Milky Way

The bimodal [Mg/Fe] versus [Fe/H] bulge sequence as revealed by APOGEE DR14

H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia

Globular cluster candidates in the Galactic bulge: Gaia and VVV view of the latest discoveries

The origin of stellar populations in the Galactic bulge from chemical abundances

The chemistry of stars in the bar of the Milky Way

Using classical Cepheids to study the far side of the Milky Way disk. I. Spectroscopic classification and the metallicity gradient

Cool stars in the Galactic center as seen by APOGEE. M giants, AGB stars, and supergiant stars and candidates

How many components? Quantifying the complexity of the metallicity distribution in the Milky Way bulge with APOGEE

The diffuse interstellar band around 8620 Å. I. Methods and application to the GIBS data set

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