JWST Spectra of Brown Dwarf Candidates in the Orion Nebula Cluster
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arXiv
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866916826245496832 |
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| author | Luhman, K. L. |
| author_facet | Luhman, K. L. |
| contents | I present an analysis of archival spectra of 200 sources toward the Orion Nebula Cluster (ONC) that were obtained with the Near-Infrared Spectrograph (NIRSpec) on board the James Webb Space Telescope (JWST). I have used these data to assess cluster membership and measure spectral types for the targets. Fifty-three sources are classified as likely cluster members, 24 of which have spectral types that are suggestive of brown dwarfs ($>$M6). Seven of the NIRSpec targets were previously identified as "Jupiter-mass binary objects" (JuMBOs), all of which are background sources rather than brown dwarfs based on the NIRSpec data. The spectral classifications of those objects are consistent with the results of my recent study of the JWST photometry in the ONC, which found that only a few JuMBO components have the colors expected for brown dwarfs, none of which form pairs that have uniquely wide separations or low masses relative to known binary brown dwarfs. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_03679 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | JWST Spectra of Brown Dwarf Candidates in the Orion Nebula Cluster Luhman, K. L. Astrophysics of Galaxies Earth and Planetary Astrophysics I present an analysis of archival spectra of 200 sources toward the Orion Nebula Cluster (ONC) that were obtained with the Near-Infrared Spectrograph (NIRSpec) on board the James Webb Space Telescope (JWST). I have used these data to assess cluster membership and measure spectral types for the targets. Fifty-three sources are classified as likely cluster members, 24 of which have spectral types that are suggestive of brown dwarfs ($>$M6). Seven of the NIRSpec targets were previously identified as "Jupiter-mass binary objects" (JuMBOs), all of which are background sources rather than brown dwarfs based on the NIRSpec data. The spectral classifications of those objects are consistent with the results of my recent study of the JWST photometry in the ONC, which found that only a few JuMBO components have the colors expected for brown dwarfs, none of which form pairs that have uniquely wide separations or low masses relative to known binary brown dwarfs. |
| title | JWST Spectra of Brown Dwarf Candidates in the Orion Nebula Cluster |
| topic | Astrophysics of Galaxies Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2507.03679 |