A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster

Abstract We present a comprehensive spectroscopic census of the Orion Nebula Cluster (ONC), based primarily on low-resolution optical spectroscopy obtained with MMT/Hectospec. We derive spectral types, youth indicators, and accretion diagnostics for 1513 stars located in the ONC region, enabling the identification and characterization of pre–main-sequence stars. We combine these measurements with a kinematic membership analysis based on Gaia Data Release 3 astrometry to identify and confirm cluster members. Using these combined diagnostics, we identify and characterize 780 bona fide T Tauri stars associated with the ONC. In addition, we construct a census of protoplanetary discs using infrared photometry obtained with the IRAC and MIPS instruments aboard the Spitzer Space Telescope. We further derive stellar masses, ages, and extinctions using the MassAge code, which combines photometric and spectroscopic inputs with stellar evolutionary models, and employs a Monte Carlo approach for uncertainty propagation. The resulting homogeneous catalogue of ONC members provides spectroscopic characterizations, kinematic membership constraints, disc diagnostics, and self-consistent estimates of stellar physical parameters. This dataset offers a refined view of the stellar population of the ONC and provides a robust foundation for investigating its kinematic structure, age distribution, and protoplanetary disc population.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-10-31
DOI
https://doi.org/10.1093/mnras/stag2013
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster

Javier Ballesteros‐Paredes, Karina Maucó, Maria Gracia Batista, L. Adame et al.
Monthly Notices of the Royal Astronomical Society
Astrophysics and Star Formation Studies
article

A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster

Javier Ballesteros‐Paredes, Karina Maucó, Maria Gracia Batista, L. Adame, Javier Serna, Alejandro Alfonso, Andrea Bonilla-Barroso, Jesús Hernández, Giovanni Pinzón, Ezequiel Manzo-Martínez, Nuria Calvet, J. J. Tobin, Lori Allen, David Fernández, Sergio Sánchez-Sanjuán, Cesar Briceno, Fabián Ahumada, Carlos Román-Zúñiga, Corina Zepeda, Luisa Zamudio-Ruvalcaba, Jhordan Peña, Johana Contreras, Lucia Martinez, Tom Megeath
article en

Abstract

Abstract We present a comprehensive spectroscopic census of the Orion Nebula Cluster (ONC), based primarily on low-resolution optical spectroscopy obtained with MMT/Hectospec. We derive spectral types, youth indicators, and accretion diagnostics for 1513 stars located in the ONC region, enabling the identification and characterization of pre–main-sequence stars. We combine these measurements with a kinematic membership analysis based on Gaia Data Release 3 astrometry to identify and confirm cluster members. Using these combined diagnostics, we identify and characterize 780 bona fide T Tauri stars associated with the ONC. In addition, we construct a census of protoplanetary discs using infrared photometry obtained with the IRAC and MIPS instruments aboard the Spitzer Space Telescope. We further derive stellar masses, ages, and extinctions using the MassAge code, which combines photometric and spectroscopic inputs with stellar evolutionary models, and employs a Monte Carlo approach for uncertainty propagation. The resulting homogeneous catalogue of ONC members provides spectroscopic characterizations, kinematic membership constraints, disc diagnostics, and self-consistent estimates of stellar physical parameters. This dataset offers a refined view of the stellar population of the ONC and provides a robust foundation for investigating its kinematic structure, age distribution, and protoplanetary disc population.

Monthly Notices of the Royal Astronomical Society
Boston University (US), Universidad de Los Andes (CO), Pedagogical and Technological University of Colombia (CO), National Radio Astronomy Observatory (US), University of Michigan (US), Universidad Nacional de Colombia (CO), Southern Astrophysical Research Telescope (CL), NSF NOIRLab (US), University of La Serena (CL), University of Oklahoma (US), Universidad Nacional Autónoma de México (MX), University of Toledo (US)
Openalex Percentile: Top 17%
Astrophysics and Star Formation Studies
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