The PHANGS-MUSE/HST-Halpha Nebulae Catalogue

Fuente: arXiv
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Hauptverfasser: Barnes, A. T., Chandar, R., Kreckel, K., Belfiore, F., Pathak, D., Thilker, D., Leroy, A. K., Groves, B., Glover, S. C. O., McClain, R., Amiri, A., Bazzi, Z., Boquien, M., Congiu, E., Dale, D. A., Egorov, O. V., Emsellem, E., Grasha, K., Lobos, J. Gonzalez, Henny, K., He, H., Indebetouw, R., Lee, J. C., Li, J., Liang, F. -H., Larson, K., Maschmann, D., Meidt, S. E., Méndez-Delgado, J. E., Neumann, J., Pan, H. -A., Querejeta, M., Rosolowsky, E., Sarbadhicary, S. K., Scheuermann, F., Úbeda, L., Williams, T. G., Weinbeck, T. D., Whitmore, B., Wofford, A., collaboration, the PHANGS
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Veröffentlicht: 2025
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author Barnes, A. T.
Chandar, R.
Kreckel, K.
Belfiore, F.
Pathak, D.
Thilker, D.
Leroy, A. K.
Groves, B.
Glover, S. C. O.
McClain, R.
Amiri, A.
Bazzi, Z.
Boquien, M.
Congiu, E.
Dale, D. A.
Egorov, O. V.
Emsellem, E.
Grasha, K.
Lobos, J. Gonzalez
Henny, K.
He, H.
Indebetouw, R.
Lee, J. C.
Li, J.
Liang, F. -H.
Larson, K.
Maschmann, D.
Meidt, S. E.
Méndez-Delgado, J. E.
Neumann, J.
Pan, H. -A.
Querejeta, M.
Rosolowsky, E.
Sarbadhicary, S. K.
Scheuermann, F.
Úbeda, L.
Williams, T. G.
Weinbeck, T. D.
Whitmore, B.
Wofford, A.
collaboration, the PHANGS
author_facet Barnes, A. T.
Chandar, R.
Kreckel, K.
Belfiore, F.
Pathak, D.
Thilker, D.
Leroy, A. K.
Groves, B.
Glover, S. C. O.
McClain, R.
Amiri, A.
Bazzi, Z.
Boquien, M.
Congiu, E.
Dale, D. A.
Egorov, O. V.
Emsellem, E.
Grasha, K.
Lobos, J. Gonzalez
Henny, K.
He, H.
Indebetouw, R.
Lee, J. C.
Li, J.
Liang, F. -H.
Larson, K.
Maschmann, D.
Meidt, S. E.
Méndez-Delgado, J. E.
Neumann, J.
Pan, H. -A.
Querejeta, M.
Rosolowsky, E.
Sarbadhicary, S. K.
Scheuermann, F.
Úbeda, L.
Williams, T. G.
Weinbeck, T. D.
Whitmore, B.
Wofford, A.
collaboration, the PHANGS
contents We present the PHANGS-MUSE/HST-Halpha nebulae catalogue, comprising 5177 spatially resolved nebulae across 19 nearby star-forming galaxies (< 20 Mpc), based on high-resolution Halpha imaging from HST, homogenised to a fixed 10 pc resolution and sensitivity. Combined with MUSE spectroscopy, this enables robust classification of 4882 H II regions and separation of planetary nebulae and supernova remnants. Electron densities for 2544 H II regions are derived using [S II] diagnostics, and nebular sizes measured via circularised radii and second moments yield a median of 20 pc, extending to sub-parsec scales. A structural complexity score traces substructure, showing that about a third of regions are H II complexes, with a higher fraction in galaxy centres. A luminosity-size relation calibrated from the HST sample is applied to 30,790 MUSE nebulae, recovering sizes down to 1 pc. Observed sizes exceed classical Stromgren radii, implying typical volume filling factors of 0.22. We associate 3349 H II regions with stellar populations from PHANGS-HST, finding median ages of 3 Myr and masses of 4-5 log(Msun). The dataset provides a detailed, spatially resolved link between nebular structure and ionising sources, serving as a benchmark for future studies of feedback, diffuse ionised gas, and star formation regulation in the interstellar medium. The full catalogue is made publicly available in machine-readable format.
format Preprint
id arxiv_https___arxiv_org_abs_2510_11778
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The PHANGS-MUSE/HST-Halpha Nebulae Catalogue
Barnes, A. T.
Chandar, R.
Kreckel, K.
Belfiore, F.
Pathak, D.
Thilker, D.
Leroy, A. K.
Groves, B.
Glover, S. C. O.
McClain, R.
Amiri, A.
Bazzi, Z.
Boquien, M.
Congiu, E.
Dale, D. A.
Egorov, O. V.
Emsellem, E.
Grasha, K.
Lobos, J. Gonzalez
Henny, K.
He, H.
Indebetouw, R.
Lee, J. C.
Li, J.
Liang, F. -H.
Larson, K.
Maschmann, D.
Meidt, S. E.
Méndez-Delgado, J. E.
Neumann, J.
Pan, H. -A.
Querejeta, M.
Rosolowsky, E.
Sarbadhicary, S. K.
Scheuermann, F.
Úbeda, L.
Williams, T. G.
Weinbeck, T. D.
Whitmore, B.
Wofford, A.
collaboration, the PHANGS
Astrophysics of Galaxies
We present the PHANGS-MUSE/HST-Halpha nebulae catalogue, comprising 5177 spatially resolved nebulae across 19 nearby star-forming galaxies (< 20 Mpc), based on high-resolution Halpha imaging from HST, homogenised to a fixed 10 pc resolution and sensitivity. Combined with MUSE spectroscopy, this enables robust classification of 4882 H II regions and separation of planetary nebulae and supernova remnants. Electron densities for 2544 H II regions are derived using [S II] diagnostics, and nebular sizes measured via circularised radii and second moments yield a median of 20 pc, extending to sub-parsec scales. A structural complexity score traces substructure, showing that about a third of regions are H II complexes, with a higher fraction in galaxy centres. A luminosity-size relation calibrated from the HST sample is applied to 30,790 MUSE nebulae, recovering sizes down to 1 pc. Observed sizes exceed classical Stromgren radii, implying typical volume filling factors of 0.22. We associate 3349 H II regions with stellar populations from PHANGS-HST, finding median ages of 3 Myr and masses of 4-5 log(Msun). The dataset provides a detailed, spatially resolved link between nebular structure and ionising sources, serving as a benchmark for future studies of feedback, diffuse ionised gas, and star formation regulation in the interstellar medium. The full catalogue is made publicly available in machine-readable format.
title The PHANGS-MUSE/HST-Halpha Nebulae Catalogue
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2510.11778