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20092026
most citedOrbitally modulated dust formation by the WC7+O5 colliding-wind binary WR140

60 citations · 267 across the 15 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2022★ 15 cited

Stellar Properties for a Comprehensive Collection of Star Forming Regions in the SDSS APOGEE-2 Survey

Carlos G. Román-Zúñiga, Marina Kounkel, Jesús Hernández +25

The Sloan Digital Sky Survey IV (SDSS-IV) APOGEE-2 primary science goal was to observe red giant stars throughout the Galaxy to study its dynamics, morphology, and chemical evoluti…

astro-ph.GA2020★ 1 cited

An infrared study of the high-mass, multi-stage star-forming region IRAS~12272-6240

Mauricio Tapia, Paolo Persi, Miguel Roth +1

IRAS 12272-6240 is a complex star forming region with a compact massive dense clump and several associated masers, located at a well-determined distance of kpc from the Sun…

astro-ph.GA2018★ 12 cited

Evidence of Hubble flow-like motion of young stellar populations away from the Perseus arm

Carlos Román-Zúñiga, Alexandre Roman-Lopes, Mauricio Tapia +2

In this letter we present evidence of coherent outward motion of a sample of young stars (30 Myr) in the Perseus Arm, whose apparent origin is located in the vicinity of the W3…

astro-ph.GA2018★ 17 cited

Massive stars in the SDSS-IV/APOGEE SURVEY. I- OB stars

A. Roman-Lopes, C. RomÁn-ZÚÑiga, Mauricio Tapia +10

In this work we make use of DR14 APOGEE spectroscopic data to study a sample of 92 known OB stars. We developed a near-infrared semi-empirical spectral classification method that w…

astro-ph.GA2017★ 9 cited

The richness of compact radio sources in NGC 6334D to F

S. -N. X. Medina, S. A. Dzib, M. Tapia +2

The presence and properties of compact radio sources embedded in massive star-forming regions can reveal important physical properties about these regions and the processes occurri…

astro-ph.GA2014★ 7 cited

The Peculiar Radio Source M17 JVLA 35

L. F. Rodriguez, C. Carrasco-Gonzalez, G. Montes +1

M17 JVLA 35 is a radio source detected in projection against the M17 HII region. In recent observations, its spectrum between 4.96 and 8.46 GHz was found to be positive and very st…