activity
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

collaborators

15 papers

astro-ph.IM2026

TESSExtractor: A web-based interactive tool for light-curve visualisation and period estimation using TESS full-frame images

Javier Serna, Jesús Hernández, Sean P. Matt +23

We present a user-friendly web application that allows users to extract, visualise, and interact with TESS light-curves (LCs) from full-frame images. The service works for any star…

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.SR2021★ 51 cited

Stellar Rotation of T Tauri stars in the Orion Star-Forming Complex

Javier Serna, Jesús Hernández, Marina Kounkel +14

We present a large-scale study of stellar rotation for T Tauri stars in the Orion Star-Forming Complex. We use the projected rotational velocity () estimations reported b…

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.SR2017★ 22 cited

New Low-Mass Stars in the 25 Orionis Stellar Group and Orion OB1a Sub-association from SDSS-III/BOSS Spectroscopy

Genaro Suárez, Juan José Downes, Carlos Román-Zúñiga +6

The Orion OB1a sub-association is a rich low mass star (LMS) region. Previous spectroscopic studies have confirmed 160 LMSs in the 25 Orionis stellar group (25 Ori), which is the m…

astro-ph.SR2015★ 32 cited

Star Formation Across the W3 Complex

C. G. Román-Zúñiga, J. Ybarra, G. Megias +3

We present a multi-wavelength analysis of the history of star formation in the W3 complex. Using deep, near-infrared ground-based images, combined with images obtained with Spitzer…

astro-ph.SR2014★ 10 cited

Spitzer IRAC Color Diagnostics for Extended Emission in Star Forming Regions

Jason E. Ybarra, Mauricio Tapia, Carlos G. Román-Zúñiga +1

The infrared data from the Spitzer Space Telescope has provided an invaluable tool for identifying physical processes in star formation. In this study we calculate the IRAC color s…

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…

astro-ph.SR2014

Periodic Radio Continuum Emission Associated with the beta Cephei Star V2187 Cyg

Mauricio Tapia, Luis F. Rodriguez, Gagik Tovmassian +4

We present new optical time-resolved photometry and medium-resolution spectroscopy of V2187 Cyg. We confirm its classification as a beta Cephei star based on sinusoidal light varia…

astro-ph.SR2011

Extended Non-Thermal Emission Possibly Associated with Cyg OB2 #5

G. N. Ortiz-Leon, L. F. Rodriguez, M. Tapia

Cyg OB2 #5 is a contact binary system (O6.5-7+O5.5-6) with associated radio continuum emission. Two compact () radio continuum components have been reported previ…

astro-ph.SR2010★ 31 cited

SDSS J123813.73-033933.0, a cataclysmic variable evolved beyond the period minimum

A. Aviles, S. Zharikov, G. Tovmassian +12

We present infrared JHK photometry of the cataclysmic variable SDSS J123813.73-033933.0 (SDSS1238)and analyze it along with optical spectroscopy, demonstrating that the binary syst…

astro-ph.SR2009★ 60 cited

Orbitally modulated dust formation by the WC7+O5 colliding-wind binary WR140

P. M. Williams, S. V. Marchenko, A. P. Marston +6

We present high-resolution infrared (2--18 micron) images of the archetypal periodic dust-making Wolf-Rayet binary system WR140 (HD 193793) taken between 2001 and 2005, and multi-c…