XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105
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| Autores principales: | , , , , , , , , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| author | Miller, Jon M. Gu, Liyi Raymond, John Brenneman, Laura Gallo, Elena Gandhi, Poshak Kallman, Timothy Kobayashi, Shogo Mao, Junjie Rogantini, Daniele Shidatsu, Megumi Ueda, Yoshihiro Xiang, Xin Zoghbi, Abderahmen |
| author_facet | Miller, Jon M. Gu, Liyi Raymond, John Brenneman, Laura Gallo, Elena Gandhi, Poshak Kallman, Timothy Kobayashi, Shogo Mao, Junjie Rogantini, Daniele Shidatsu, Megumi Ueda, Yoshihiro Xiang, Xin Zoghbi, Abderahmen |
| contents | GRS 1915$+$105 was the stellar-mass black hole that best reproduced key phenomena that are also observed in Type-1 active galactic nuclei. In recent years, however, it has evolved to resemble a Type-2 or Compton-thick AGN. Herein, we report on the first XRISM observation of GRS 1915$+$105. The high-resolution Resolve calorimeter spectrum reveals that a sub-Eddington central engine is covered by a layer of warm, Compton-thick gas. With the obscuration acting as a coronagraph, numerous strong, narrow emission lines from He-like and H-like charge states of Si, S, Ar, Ca, Cr, Mn, Fe, and Ni dominate the spectrum. Radiative recombination continuum (RRC) features are also observed, signaling that much of the emitting gas is photoionized. The line spectrum can be fit by three photoionized emission zones, with broadening and bulk velocities suggestive of an origin in the outer disk atmosphere and/or a slow wind at $r \simeq 10^{6}~GM/c^{2}$. The Fe XXV He-$α$ and Fe XXVI Ly-$α$ lines have a broad base that may indicate some emission from $r \sim 3\times 10^{3}~GM/c^{2}$. These results broadly support a picture wherein the current state in GRS 1915$+$105 is due to obscuration by the irradiated outer disk. This could arise through disk thickening if the Eddington fraction is higher than inferred, but it is more likely due to a warped, precessing disk that has brought the outer disk into the line of sight. We discuss the strengths and weaknesses of this interpretation and our modeling, and possible explanations of some potentially novel spectral features. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2510_25089 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105 Miller, Jon M. Gu, Liyi Raymond, John Brenneman, Laura Gallo, Elena Gandhi, Poshak Kallman, Timothy Kobayashi, Shogo Mao, Junjie Rogantini, Daniele Shidatsu, Megumi Ueda, Yoshihiro Xiang, Xin Zoghbi, Abderahmen High Energy Astrophysical Phenomena GRS 1915$+$105 was the stellar-mass black hole that best reproduced key phenomena that are also observed in Type-1 active galactic nuclei. In recent years, however, it has evolved to resemble a Type-2 or Compton-thick AGN. Herein, we report on the first XRISM observation of GRS 1915$+$105. The high-resolution Resolve calorimeter spectrum reveals that a sub-Eddington central engine is covered by a layer of warm, Compton-thick gas. With the obscuration acting as a coronagraph, numerous strong, narrow emission lines from He-like and H-like charge states of Si, S, Ar, Ca, Cr, Mn, Fe, and Ni dominate the spectrum. Radiative recombination continuum (RRC) features are also observed, signaling that much of the emitting gas is photoionized. The line spectrum can be fit by three photoionized emission zones, with broadening and bulk velocities suggestive of an origin in the outer disk atmosphere and/or a slow wind at $r \simeq 10^{6}~GM/c^{2}$. The Fe XXV He-$α$ and Fe XXVI Ly-$α$ lines have a broad base that may indicate some emission from $r \sim 3\times 10^{3}~GM/c^{2}$. These results broadly support a picture wherein the current state in GRS 1915$+$105 is due to obscuration by the irradiated outer disk. This could arise through disk thickening if the Eddington fraction is higher than inferred, but it is more likely due to a warped, precessing disk that has brought the outer disk into the line of sight. We discuss the strengths and weaknesses of this interpretation and our modeling, and possible explanations of some potentially novel spectral features. |
| title | XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2510.25089 |