Resolving the Multiple Component Outflows in PG 1211+143. I. The Fe–K Absorption Structure and UFO Forest
Indexed incrossrefdoaj
Abstract
Abstract We present the initial high-resolution X-ray spectroscopic observations of the Fe–K absorption structure in the luminous nearby quasar PG 1211+143, utilizing the X-ray Imaging and Spectroscopy Mission (XRISM). The primary objective is to characterize the Fe–K absorption features due to ultra-fast outflow (UFO) in this Eddington-luminosity source. Observations were conducted with XRISM’s Resolve and Xtend instruments, complemented by simultaneous data from XMM-Newton and NuSTAR. A historically bright phase was captured. The Resolve spectra clearly reveal a prominent P Cygni profile and resolves the Fe–K absorption into six distinct velocity components, ranging from v = −0.074 to −0.405 c . A similar…
Citation impact
4
total citations
- FWCI
- 48.04
- Percentile
- 99%
- References
- 47
Too recent for citation history.
Authors
18Topics & keywords
Topics
Keywords
- Outflow
- Quasar
- Absorption (acoustics)
- Spectral line
- Accretion (finance)
- Spectroscopy
No related works found for this paper.
Funding
- NANational Aeronautics and Space AdministrationAwards: 80NSSC25K7845, ST/T000244/1, 80NSSC22K0474
- KUKagoshima University
- HUHirosaki University
- SAScience and Technology Facilities CouncilAwards: ST/T000244, T000244, ST/T000244/1
- JSJapan Society for the Promotion of ScienceAwards: JP20H01947, JP20K14525, JP21K13963, JP24K00672, JP24K17104, JP20H01946, JP21K13958, JP24K00638, JP20KK0071, JPJSCCA20220002, JP23K13154, JP23K20239, JP19K21884