دورية أكاديمية
Supermassive Black Hole Winds in X-rays: SUBWAYS
| العنوان: | Supermassive Black Hole Winds in X-rays: SUBWAYS |
|---|---|
| المؤلفون: | Mehdipour, M., Kriss, G. A., Brusa, M., Matzeu, G.A., Gaspari, M., Kraemer, S. B., Mathur, Savita, Behar, E., Bianchi, Stefano, Cappi, M., Chartas, G., Costantini, E., Cresci, G., Dadina, M., Marco, B. De, Rosa, A. De, Dunn, J. P., Gianolli, V. E., Miniutti, Giovanni, Kaastra, J. S., King, A. R., Krongold, Y., Franca, F. La, Lanzuisi, G., Longinotti, A. L., Luminari, A., Middei, R., G. Miniutt, Giustini, Margherita, Nardini, E., Perna, M., Petrucci, P.-O., Piconcelli, E., Ponti, G., Ricci, F., Tombesi, F., Ursini, F., Vignali, C., Zappacosta, L. |
| المساهمون: | National Aeronautics and Space Administration (US), California Institute of Technology, European Commission, Israel Science Foundation, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Comunidad de Madrid, Consejo Nacional de Ciencia y Tecnología (México), Ministerio de Economía y Competitividad (España), Centre National de la Recherche Scientifique (France), Ministero dell'Istruzione e del Merito |
| بيانات النشر: | EDP Sciences |
| سنة النشر: | 2023 |
| المجموعة: | Digital.CSIC (Consejo Superior de Investigaciones Científicas / Spanish National Research Council) |
| مصطلحات موضوعية: | Galaxies: active, Ultraviolet: galaxies, X-rays: galaxies, Techniques: spectroscopic |
| الوصف: | We present a UV spectroscopic study of ionized outflows in 21 active galactic nuclei (AGN), observed with the Hubble Space Telescope (HST). The targets of the Supermassive Black Hole Winds in X-rays (SUBWAYS) sample were selected with the aim to probe the parameter space of the underexplored AGN between the local Seyfert galaxies and the luminous quasars at high redshifts. Our targets, spanning redshifts of 0.1–0.4 and bolometric luminosities (Lbol) of 1045–1046 erg s−1, have been observed with a large multi-wavelength campaign using XMM-Newton, NuSTAR, and HST. Here, we model the UV spectra and look for different types of AGN outflows that may produce either narrow or broad UV absorption features. We examine the relations between the observed UV outflows and other properties of the AGN. We find that 60% of our targets show a presence of outflowing H I absorption, while 40% exhibit ionized outflows seen as absorption by either C IV, N V, or O VI. This is comparable to the occurrence of ionized outflows seen in the local Seyfert galaxies. All UV absorption lines in the sample are relatively narrow, with outflow velocities reaching up to −3300 km s−1. We did not detect any UV counterparts to the X-ray ultra-fast outflows (UFOs), most likely due to their being too highly ionized to produce significant UV absorption. However, all SUBWAYS targets with an X-ray UFO that have HST data demonstrate the presence of UV outflows at lower velocities. We find significant correlations between the column density (N) of the UV ions and Lbol of the AGN, with NH I decreasing with Lbol, while NO VI is increasing with Lbol. This is likely to be a photoionization effect, where toward higher AGN luminosities, the wind becomes more ionized, resulting in less absorption by neutral or low-ionization ions and more absorption by high-ionization ions. In addition, we find that N of the UV ions decreases as their outflow velocity increases. This may be explained by a mechanical power that is evacuating the UV-absorbing medium. Our observed ... |
| نوع الوثيقة: | article in journal/newspaper |
| وصف الملف: | application/pdf |
| اللغة: | English |
| تدمد: | 0004-6361 1432-0746 |
| العلاقة: | #PLACEHOLDER_PARENT_METADATA_VALUE#; info:eu-repo/grantAgreement/EC/H2020/860744; info:eu-repo/grantAgreement/AEI//IRYC2018-025950-I; info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-117252GB-I00/ES/ENANAS BLANCAS, ESTRELLAS DE NEUTRONES Y AGUJEROS NEGROS - FISICA DE LAS ESTRELLAS COMPACTAS/; 2018-T1/TIC-11733; info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-83197-P/ES/PARTICIPACION ESPAÑOLA EN EL TELESCOPIO JAMES WEBB: ACTIVIDADES PREVIAS AL LANZAMIENTO, CARACTERIZACION EN ORBITA, Y EXPLOTACION CIENTIFICA DEL TIEMPO GARANTIZADO/; info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-106280GB-I00/ES/PARTICIPACION ESPAÑOLA EN EL TELESCOPIO JAMES WEBB: ACTIVIDADES PREVIAS AL LANZAMIENTO, CARACTERIZACION EN ORBITA,Y PREPARACION DE PROGRAMAS CIENTIFICOS DE TIEMPO GARANTIZAD/; info:eu-repo/grantAgreement/EC/H2020/865637; Publisher's version; https://doi.org/10.1051/0004-6361/202245047Test; Sí; Astronomy & Astrophysics 675: A183 (2023); http://hdl.handle.net/10261/347553Test |
| DOI: | 10.1051/0004-6361/202245047 |
| الإتاحة: | https://doi.org/10.1051/0004-6361/202245047Test http://hdl.handle.net/10261/347553Test |
| حقوق: | open |
| رقم الانضمام: | edsbas.DF0E371D |
| قاعدة البيانات: | BASE |
Full Text Finder | تدمد: | 00046361 14320746 |
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| DOI: | 10.1051/0004-6361/202245047 |