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Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Kluge, M., Hatch, N. A., Montes, M., Golden-Marx, J. B., Gonzalez, A. H., Cuillandre, J. -C., Bolzonella, M., Lançon, A., Laureijs, R., Saifollahi, T., Schirmer, M., Stone, C., Boselli, A., Cantiello, M., Sorce, J. G., Marleau, F. R., Duc, P. -A., Sola, E., Urbano, M., Ahad, S. L., Bahé, Y. M., Bamford, S. P., Bellhouse, C., Buitrago, F., Dimauro, P., Durret, F., Ellien, A., Jimenez-Teja, Y., Slezak, E., Aghanim, N., Altieri, B., Andreon, S., Auricchio, N., Baldi, M., Balestra, A., Bardelli, S., Bender, R., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Candini, G. P., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castellano, M., Cavuoti, S., Cimatti, A., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Courbin, F., Courtois, H. M., Cropper, M., Da Silva, A., Degaudenzi, H., Dinis, J., Duncan, C. A. J., Dupac, X., Dusini, S., Farina, M., Farrens, S., Ferriol, S., Fosalba, P., Frailis, M., Franceschi, E., Fumana, M., Galeotta, S., Garilli, B., Gillard, W., Gillis, B., Giocoli, C., Gómez-Alvarez, P., Granett, B. R., Grazian, A., Grupp, F., Guzzo, L., Haugan, S. V. H., Hoar, J., Hoekstra, H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Hudelot, P., Jahnke, K., Keihänen, E., Kermiche, S., Kiessling, A., Kitching, T., Kohley, R., Kubik, B., Kümmel, M., Kunz, M., Kurki-Suonio, H., Lahav, O., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., McCracken, H. J., Medinaceli, E., Mei, S., Melchior, M., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Munari, E., Nichol, R. C., Niemi, S. -M., Nightingale, J. W., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Racca, G. D., Raison, F., Rebolo, R., Renzi, A., Rhodes, J., Riccio, G., Rix, H. -W., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Sartoris, B., Sauvage, M., Scaramella, R., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Seiffert, M., Serrano, S., Sirignano, C., Sirri, G., Skottfelt, J., Stanco, L., Tallada-Crespí, P., Taylor, A. N., Teplitz, H. I., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Vassallo, T., Kleijn, G. Verdoes, Veropalumbo, A., Wang, Y., Weller, J., Williams, O. R., Zamorani, G., Zucca, E., Biviano, A., Burigana, C., De Lucia, G., George, K., Scottez, V., Simon, P., Mora, A., Martín-Fleitas, J., Ruppin, F., Scott, D.
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
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_version_	1866909596232187904
author	Kluge, M. Hatch, N. A. Montes, M. Golden-Marx, J. B. Gonzalez, A. H. Cuillandre, J. -C. Bolzonella, M. Lançon, A. Laureijs, R. Saifollahi, T. Schirmer, M. Stone, C. Boselli, A. Cantiello, M. Sorce, J. G. Marleau, F. R. Duc, P. -A. Sola, E. Urbano, M. Ahad, S. L. Bahé, Y. M. Bamford, S. P. Bellhouse, C. Buitrago, F. Dimauro, P. Durret, F. Ellien, A. Jimenez-Teja, Y. Slezak, E. Aghanim, N. Altieri, B. Andreon, S. Auricchio, N. Baldi, M. Balestra, A. Bardelli, S. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. Dinis, J. Duncan, C. A. J. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Granett, B. R. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoar, J. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kohley, R. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Lahav, O. Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H. J. Medinaceli, E. Mei, S. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Racca, G. D. Raison, F. Rebolo, R. Renzi, A. Rhodes, J. Riccio, G. Rix, H. -W. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Sauvage, M. Scaramella, R. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Tallada-Crespí, P. Taylor, A. N. Teplitz, H. I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Williams, O. R. Zamorani, G. Zucca, E. Biviano, A. Burigana, C. De Lucia, G. George, K. Scottez, V. Simon, P. Mora, A. Martín-Fleitas, J. Ruppin, F. Scott, D.
author_facet	Kluge, M. Hatch, N. A. Montes, M. Golden-Marx, J. B. Gonzalez, A. H. Cuillandre, J. -C. Bolzonella, M. Lançon, A. Laureijs, R. Saifollahi, T. Schirmer, M. Stone, C. Boselli, A. Cantiello, M. Sorce, J. G. Marleau, F. R. Duc, P. -A. Sola, E. Urbano, M. Ahad, S. L. Bahé, Y. M. Bamford, S. P. Bellhouse, C. Buitrago, F. Dimauro, P. Durret, F. Ellien, A. Jimenez-Teja, Y. Slezak, E. Aghanim, N. Altieri, B. Andreon, S. Auricchio, N. Baldi, M. Balestra, A. Bardelli, S. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. Dinis, J. Duncan, C. A. J. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Granett, B. R. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoar, J. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kohley, R. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Lahav, O. Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H. J. Medinaceli, E. Mei, S. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Racca, G. D. Raison, F. Rebolo, R. Renzi, A. Rhodes, J. Riccio, G. Rix, H. -W. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Sauvage, M. Scaramella, R. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Tallada-Crespí, P. Taylor, A. N. Teplitz, H. I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Williams, O. R. Zamorani, G. Zucca, E. Biviano, A. Burigana, C. De Lucia, G. George, K. Scottez, V. Simon, P. Mora, A. Martín-Fleitas, J. Ruppin, F. Scott, D.
contents	We study the intracluster light (ICL) and intracluster globular clusters (ICGCs) in the nearby Perseus galaxy cluster using Euclid's EROs. By modelling the isophotal and iso-density contours, we mapped the distributions and properties of the ICL and ICGCs out to radii of 200-600 kpc (up to ~1/3 of the virial radius) from the brightest cluster galaxy (BCG). We find that the central 500 kpc hosts 70000$\pm$2800 GCs and $1.7\times10^{12}$ L$_\odot$ of diffuse light from the BCG+ICL in the near-infrared H$_E$. This accounts for 38$\pm$6% of the cluster's total stellar luminosity within this radius. The ICL and ICGCs share a coherent spatial distribution, suggesting a common origin or that a common potential governs their distribution. Their contours on the largest scales (>200 kpc) are offset from the BCG's core westwards by 60 kpc towards several luminous cluster galaxies. This offset is opposite to the displacement observed in the gaseous intracluster medium. The radial surface brightness profile of the BCG+ICL is best described by a double Sérsic model, with 68$\pm$4% of the H$_E$ light in the extended, outer component. The transition between these components occurs at ~60 kpc, beyond which the isophotes become increasingly elliptical and off-centred. The radial ICGC number density profile closely follows the BCG+ICL profile only beyond this 60 kpc radius, where we find an average of 60-80 GCs per $10^9$ M$_\odot$ of diffuse stellar mass. The BCG+ICL colour becomes increasingly blue with radius, consistent with the stellar populations in the ICL having subsolar metallicities [Fe/H] ~ -0.6 to -1.0. The colour of the ICL, and the specific frequency and luminosity function of the ICGCs suggest that the ICL+ICGCs were tidally stripped from the outskirts of massive satellites with masses of a few $\times10^{10}$ M$_\odot$, with an increasing contribution from dwarf galaxies at large radii.
format	Preprint
id	arxiv_https___arxiv_org_abs_2405_13503
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster Kluge, M. Hatch, N. A. Montes, M. Golden-Marx, J. B. Gonzalez, A. H. Cuillandre, J. -C. Bolzonella, M. Lançon, A. Laureijs, R. Saifollahi, T. Schirmer, M. Stone, C. Boselli, A. Cantiello, M. Sorce, J. G. Marleau, F. R. Duc, P. -A. Sola, E. Urbano, M. Ahad, S. L. Bahé, Y. M. Bamford, S. P. Bellhouse, C. Buitrago, F. Dimauro, P. Durret, F. Ellien, A. Jimenez-Teja, Y. Slezak, E. Aghanim, N. Altieri, B. Andreon, S. Auricchio, N. Baldi, M. Balestra, A. Bardelli, S. Bender, R. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Candini, G. P. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C. J. Conversi, L. Copin, Y. Courbin, F. Courtois, H. M. Cropper, M. Da Silva, A. Degaudenzi, H. Dinis, J. Duncan, C. A. J. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Fosalba, P. Frailis, M. Franceschi, E. Fumana, M. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Gómez-Alvarez, P. Granett, B. R. Grazian, A. Grupp, F. Guzzo, L. Haugan, S. V. H. Hoar, J. Hoekstra, H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Hudelot, P. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kohley, R. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Lahav, O. Ligori, S. Lilje, P. B. Lindholm, V. Lloro, I. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H. J. Medinaceli, E. Mei, S. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moresco, M. Moscardini, L. Munari, E. Nichol, R. C. Niemi, S. -M. Nightingale, J. W. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Percival, W. J. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L. A. Pozzetti, L. Racca, G. D. Raison, F. Rebolo, R. Renzi, A. Rhodes, J. Riccio, G. Rix, H. -W. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Sauvage, M. Scaramella, R. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Seiffert, M. Serrano, S. Sirignano, C. Sirri, G. Skottfelt, J. Stanco, L. Tallada-Crespí, P. Taylor, A. N. Teplitz, H. I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E. A. Valenziano, L. Vassallo, T. Kleijn, G. Verdoes Veropalumbo, A. Wang, Y. Weller, J. Williams, O. R. Zamorani, G. Zucca, E. Biviano, A. Burigana, C. De Lucia, G. George, K. Scottez, V. Simon, P. Mora, A. Martín-Fleitas, J. Ruppin, F. Scott, D. Astrophysics of Galaxies We study the intracluster light (ICL) and intracluster globular clusters (ICGCs) in the nearby Perseus galaxy cluster using Euclid's EROs. By modelling the isophotal and iso-density contours, we mapped the distributions and properties of the ICL and ICGCs out to radii of 200-600 kpc (up to ~1/3 of the virial radius) from the brightest cluster galaxy (BCG). We find that the central 500 kpc hosts 70000$\pm$2800 GCs and $1.7\times10^{12}$ L$_\odot$ of diffuse light from the BCG+ICL in the near-infrared H$_E$. This accounts for 38$\pm$6% of the cluster's total stellar luminosity within this radius. The ICL and ICGCs share a coherent spatial distribution, suggesting a common origin or that a common potential governs their distribution. Their contours on the largest scales (>200 kpc) are offset from the BCG's core westwards by 60 kpc towards several luminous cluster galaxies. This offset is opposite to the displacement observed in the gaseous intracluster medium. The radial surface brightness profile of the BCG+ICL is best described by a double Sérsic model, with 68$\pm$4% of the H$_E$ light in the extended, outer component. The transition between these components occurs at ~60 kpc, beyond which the isophotes become increasingly elliptical and off-centred. The radial ICGC number density profile closely follows the BCG+ICL profile only beyond this 60 kpc radius, where we find an average of 60-80 GCs per $10^9$ M$_\odot$ of diffuse stellar mass. The BCG+ICL colour becomes increasingly blue with radius, consistent with the stellar populations in the ICL having subsolar metallicities [Fe/H] ~ -0.6 to -1.0. The colour of the ICL, and the specific frequency and luminosity function of the ICGCs suggest that the ICL+ICGCs were tidally stripped from the outskirts of massive satellites with masses of a few $\times10^{10}$ M$_\odot$, with an increasing contribution from dwarf galaxies at large radii.
title	Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster
topic	Astrophysics of Galaxies
url	https://arxiv.org/abs/2405.13503