dorsal/arxiv
View SchemaAre Recently Quenched Ellipticals Truly Isolated Centrals?
| Authors | Deepak K. Deo |
|---|---|
| Categories | |
| ArXiv ID | 2601.09846vv1 |
| URL | https://arxiv.org/abs/2601.09846 |
| License | http://creativecommons.org/licenses/by/4.0/ |
Abstract
Recently Quenched Ellipticals (RQEs) provide a valuable test case for disentangling intrinsic and environmental quenching, particularly because they are commonly classified as isolated central galaxies in low-mass halos. However, central/satellite assignments and isolation labels can vary across group catalogs, and such misclassifications can strongly bias physical interpretations. We present a uniform, physically motivated reassessment of the environments of 155 RQEs previously identified as centrals in an SDSS-based group catalog. We construct value-added neighbor catalogs via KD-tree searches and apply consistent thresholds in projected separation and line-of-sight velocity to (i) verify centrality, (ii) quantify isolation using a mass-ratio-based companion criterion, and (iii) identify potential pseudo-centrals via proximity to massive clusters. We find that 132/155 (85.2\%) RQEs remain true centrals, while 23/155 (14.8\%) are better interpreted as misidentified centrals with a more massive neighbor within $R_{\rm proj}\leq0.8$~Mpc and $\Delta V\leq250$~km~s$^{-1}$. Among the true centrals, 110/132 (83.3\%) satisfy our isolation criterion, and only one system meets our pseudo-central definition, indicating that direct cluster-scale preprocessing is rare for RQE centrals. Using projected number density and surface stellar mass density, we show that misidentified and non-isolated systems occupy systematically denser regimes than isolated true centrals. These results imply that while most RQEs ($\sim$71\%) are consistent with predominantly internal quenching in genuinely isolated centrals, a non-negligible minority ($\sim$29\%) likely experienced environmentally influenced pathways at group scales.
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"abstract": "Recently Quenched Ellipticals (RQEs) provide a valuable test case for disentangling intrinsic and environmental quenching, particularly because they are commonly classified as isolated central galaxies in low-mass halos. However, central/satellite assignments and isolation labels can vary across group catalogs, and such misclassifications can strongly bias physical interpretations. We present a uniform, physically motivated reassessment of the environments of 155 RQEs previously identified as centrals in an SDSS-based group catalog. We construct value-added neighbor catalogs via KD-tree searches and apply consistent thresholds in projected separation and line-of-sight velocity to (i) verify centrality, (ii) quantify isolation using a mass-ratio-based companion criterion, and (iii) identify potential pseudo-centrals via proximity to massive clusters. We find that 132/155 (85.2\\%) RQEs remain true centrals, while 23/155 (14.8\\%) are better interpreted as misidentified centrals with a more massive neighbor within $R_{\\rm proj}\\leq0.8$~Mpc and $\\Delta V\\leq250$~km~s$^{-1}$. Among the true centrals, 110/132 (83.3\\%) satisfy our isolation criterion, and only one system meets our pseudo-central definition, indicating that direct cluster-scale preprocessing is rare for RQE centrals. Using projected number density and surface stellar mass density, we show that misidentified and non-isolated systems occupy systematically denser regimes than isolated true centrals. These results imply that while most RQEs ($\\sim$71\\%) are consistent with predominantly internal quenching in genuinely isolated centrals, a non-negligible minority ($\\sim$29\\%) likely experienced environmentally influenced pathways at group scales.",
"arxiv_id": "2601.09846",
"authors": [
"Deepak K. Deo"
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"astro-ph.GA"
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"license": "http://creativecommons.org/licenses/by/4.0/",
"title": "Are Recently Quenched Ellipticals Truly Isolated Centrals?",
"url": "https://arxiv.org/abs/2601.09846",
"version": "v1"
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