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20052026
most citedThe SDSS-III APOGEE Spectral Line List for H-band Spectroscopy

172 citations · 1.1k across the 25 of their papers we have counts for

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astro-ph.SR2023★ 8 cited

Chemical abundances of the young inner-disk open cluster NGC 6705 observed by APOGEE: sodium-rich and not -enhanced

V. Loaiza-Tacuri, K. Cunha, D. Souto +19

Previous results in the literature have found the young inner-disk open cluster NGC 6705 to be mildly -enhanced. We examined this possibility via an independent chemical abundan…

astro-ph.SR2022

Confirmation of the star J004229.87+410551.8 in M31 as a B[e] supergiant

Sarkisyan A., Vinokurov A., Solovyeva Yu. +4

We study the luminous blue variable candidate J004229.87+410551.8 in the Andromeda Galaxy. Earlier, the star displayed a spectral anomaly: although a hot emission spectrum had been…

astro-ph.SR2022★ 5 cited

Search for LBVs in the Local Volume galaxies: study of four stars in NGC 4449

Y. Solovyeva, A. Vinokurov, A. Sarkisyan +8

We continue to search for LBV stars in galaxies outside the Local Group. In this work, we have investigated four luminous stars in NGC 4449. Multiple spectral observations carried…

astro-ph.SR2020★ 8 cited

Modeling spectra of MN112

A. Kostenkov, S. Fabrika, O. Sholukhova +2

MN112 is the Galactic luminous blue variable (LBV) candidate with circumstellar nebula. P Cygni is the first discovered LBV, which was recorded during major eruptions in the 17th c…

astro-ph.SR2020★ 9 cited

Luminous Blue Variable candidates in M31

A. Sarkisyan, O. Sholukhova, S. Fabrika +7

We study five Luminous Blue Variable (LBV) candidates in the Andromeda galaxy and one more (MN112) in the Milky Way. We obtain the same-epoch near-infrared (NIR) and optical spectr…

astro-ph.SR2016★ 32 cited

Chemical Abundances in a Sample of Red Giants in the Open Cluster NGC 2420 from APOGEE

Diogo Souto, Katia Cunha, Verne Smith +20

NGC 2420 is a 2 Gyr-old well-populated open cluster that lies about 2 kpc beyond the solar circle, in the general direction of the Galactic anti-center. Most previous abundan…