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Bipolar Hypershell Galactic Center Starburst Model: Further Evidence from ROSAT Data and New Radio and X‐Ray Simulations
Open accessAbstract
Using the all-sky ROSAT soft X-ray and 408 MHz radio continuum data, we show that the North Polar Spur (NPS) and its western and southern counterspurs draw a giant dumbbell shape necked at the Galactic plane. We interpret these features as due to a shock front originating from a starburst 15 million years ago with a total energy of the order of ~10 56 ergs or 10 5 Type II supernovae. We simulate all-sky distributions of radio continuum and soft X-ray intensities based on the bipolar hypershell Galactic center starburst model. The simulations can well reproduce the radio NPS and related spurs, as well as radio spurs in the tangential directions of spiral arms. Simulated X-ray maps in the 0.25, 0.75, and 1.5 keV bands reproduce the ROSAT X-ray NPS, its western and southern counterspurs, and the absorption layer along the Galactic plane. We propose to use the ROSAT all-sky maps to probe the physics of gas in the halo-intergalactic interface, and to directly date and measure the energy of a recent Galactic center starburst.
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“The energy requirement for the X-shaped region is ∼ 10 55 erg (Bland-Hawthorn & Cohen 2003), about an order of magnitude smaller than the required energy of ∼ 10 56 erg for the eROSITA bubbles (Sofue 2000; Kataoka et al. 2013; Predehl et al. 2021).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Sofue 2000
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Cites
Interstellar photoelectric absorption cross sections, 0.03-10 keV
Morrison, R., & McCammon, D. (1983) · The Astrophysical Journal · doi:10.1086/161102 · Cited by 1,755
On the nature and implications of starburst-driven galactic superwinds
Heckman, T. M., Armus, L., & MILEY, G. K. (1990) · The Astrophysical Journal Supplement Series · doi:10.1086/191522 · Cited by 1,158
Ghez, A. M., Klein, B., Morris, M., & Becklin, E. E. (1998) · The Astrophysical Journal · doi:10.1086/306528 · Cited by 770
ROSAT Survey Diffuse X‐Ray Background Maps. II.
Snowden, S. L., Egger, R., Freyberg, M. J., McCammon, D., Plucinsky, P. P., Sanders, W. T., Schmitt, J. H. M. M., Trumper, J., & Voges, W. (1997) · The Astrophysical Journal · doi:10.1086/304399 · Cited by 602 · cited 10×
“Snowden et al. (1997) have further noticed cylindrical features in the R45 and R67 (1.5 keV) band maps, which emerge from the central Galactic disk toward the halo.”
BackgroundMethodInfluentialAtlas of Galactic Neutral Hydrogen
Hartmann, D., Burton, W. B., & Kerr, F. J. (1998) · Physics Today · doi:10.1063/1.882290 · Cited by 425
On the nature of the dark mass in the centre of the Milky Way
Genzel, R., Eckart, A., Ott, T., & Eisenhauer, F. (1997) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/291.1.219 · Cited by 352
The soft X-ray diffuse background
McCammon, D., Burrows, D. N., Sanders, W. T., III, & Kraushaar, W. L. (1983) · The Astrophysical Journal · doi:10.1086/161024 · Cited by 232
The Soft X-Ray Background and Its Origins
McCammon, D., & Sanders, W. T., III (1990) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.28.090190.003301 · Cited by 217
The nuclear superbubble of NGC 3079
Veilleux, S., Cecil, G. N., Bland‐Hawthorn, J., Tully, R. B., Filippenko, A. V., & Sargent, W. L. W. (1994) · The Astrophysical Journal · doi:10.1086/174624 · Cited by 164
Interstellar extinction from infrared to X-rays: An overview
Ryter, C. E. (1996) · Astrophysics and Space Science · doi:10.1007/bf00645150 · Cited by 151
Flagged first, then by citations
Research works printed but not linked: 17
- Berkhuijsen E., 1971, A&A, 14, 252
- Egger, R. 1993, Ph.D. thesis, Univ. Munich
- Egger R. J., 1995, A&A, 294, L25
- Haslam C. G. T., 1982, A&AS, 47, 1
- Mollenhoff C., 1976, A&A, 50, 105
- Nakai N., 1992, PASJ, 44, L27
- Nakai N., 1987, PASJ, 39, 685
- Oort J. H., 1977, ARA&A, 15, 259
- Pietsch W., 1998, A&A, 340, 351
- Pietsch, W., Vogler, A., Klein, U. & Zinnecker, H. 2000, A&A, in press
- Sofue Y., 1976, A&A, 48, 1
- Sofue Y., 1977, A&A, 60, 327
- Sofue Y., 1984, PASJ, 36, 539
- Sofue Y., 1979, A&AS, 38, 251
- van Albada G. D., 1982, A&A, 115, 263
- Vogler A., 1999, A&A, 342, 101
- Vogler A., 1999, A&A, 352, 64
Cited by
Sorted by citations
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Su, M., Slatyer, T., & Finkbeiner, D. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/724/2/1044 · Cited by 756
Quasar feedback and the origin of radio emission in radio-quiet quasars
Zakamska, N. L., & Greene, J. E. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu842 · Cited by 360
The Large‐Scale Bipolar Wind in the Galactic Center
Bland‐Hawthorn, J., & Cohen, M. (2003) · The Astrophysical Journal · doi:10.1086/344573 · Cited by 301
Detection of large-scale X-ray bubbles in the Milky Way halo
Predehl, P., Sunyaev, R. A., Becker, W., Brunner, H., Burenin, R., Bykov, A., Cherepashchuk, A., Chugai, N., Churazov, E., Doroshenko, V., et al. (2020) · Nature · doi:10.1038/s41586-020-2979-0 · Cited by 234
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Guo, F., & Mathews, W. G. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/756/2/181 · Cited by 231
A faint discrete source origin for the highly ionized iron emission from the Galactic Centre region
Wang, Q. D., Gotthelf, E. V., & Lang, C. (2002) · Nature · doi:10.1038/415148a · Cited by 194
Detection of large-scale X-ray bubbles in the Milky Way halo
Predehl, P., Sunyaev, R., Becker, W., Brunner, H., Burenin, R., Bykov, A. M., Cherepashchuk, A. M., Чугай, Н. Н., Churazov, E., Doroshenko, V., et al. (2020) · RePEc: Research Papers in Economics · Cited by 188
Wild at Heart:-The Particle Astrophysics of the Galactic Centre
Crocker, R., Jones, D., Aharonian, F., Law, C., Melia, F., Oka, T., & Ott, J. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18170.x · Cited by 107
Crocker, R. M., Bicknell, G. V., Taylor, A. M., & Carretti, E. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/808/2/107 · Cited by 120
“It has long been argued on the basis of stellar polarization data that the NPS is a structure of the local ISM (within a few × 102 pc; Bingham 1967; Berkhuijsen et al. 1971).”
BackgroundResultInfluentialSUZAKU OBSERVATIONS OF THE DIFFUSE X-RAY EMISSION ACROSS THE FERMI BUBBLES' EDGES
Kataoka, J., Tahara, M., Totani, T., Sofue, Y., Stawarz, Ł., Takahashi, Y., Takeuchi, Y., Tsunemi, H., Kimura, M., Takei, Y., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/779/1/57 · Cited by 118
Self-citationFERMI BUBBLES INFLATED BY WINDS LAUNCHED FROM THE HOT ACCRETION FLOW IN SGR A*
Mou, G., Yuan, F., Bu, D., Sun, M., & Su, M. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/790/2/109 · Cited by 97
“…Center Lobe (GCL, Bland-Hawthorn & Cohen 2003); 5) Expanding Molecular Ring (EMR, Kaifu et al. 1972; Scoville 1972); 6) North Polar Spur (NPS, Sofue 2000; Bland-Hawthorn & Cohen 2003); 7) the 8 keV diffuse X-ray emission in the center (Muno et al. 2004); 8) the excess of Hα emission of…”
BackgroundTotani, T. (2006) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/58.6.965 · Cited by 80
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Miller, M. J., & Bregman, J. N. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/829/1/9 · Cited by 91
Crocker, R. M. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21149.x · Cited by 88
The Fermi bubbles as starburst wind termination shocks
Lacki, B. C. (2014) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slu107 · Cited by 79
Fermi and eROSITA bubbles as relics of the past activity of the Galaxy’s central black hole
Yang, H.-Y. K., Ruszkowski, M., & Zweibel, E. G. (2022) · Nature Astronomy · doi:10.1038/s41550-022-01618-x · Cited by 68
The High‐Velocity Gas toward Messier 5: Tracing Feedback Flows in the Inner Galaxy
Zech, W. F., Lehner, N., Howk, J. C., Van Dyke Dixon, W., & Brown, T. M. (2008) · The Astrophysical Journal · doi:10.1086/587135 · Cited by 61
Abundance and temperature of the outer hot circumgalactic medium
Ponti, G., Zheng, X., Locatelli, N. T., Bianchi, S., Zhang, Y., Anastasopoulou, K., Comparat, J., Dennerl, K., Freyberg, M. J., Haberl, F., et al. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243992 · Cited by 59
X-ray and Gamma-ray Observations of the Fermi Bubbles and NPS/Loop I Structures
Kataoka, J., Sofue, Y., Inoue, Y., Akita, M., Nakashima, S., & Totani, T. (2018) · Galaxies · doi:10.3390/galaxies6010027 · Cited by 43
Self-citationSun, X. H., Landecker, T. L., Gaensler, B. M., Carretti, E., Reich, W., Leahy, J. P., McClure-Griffiths, N. M., Crocker, R. M., Wolleben, M., Haverkorn, M., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/811/1/40 · Cited by 53
The X-ray spectrum of the North Polar Spur
Willingale, R., Hands, A. D. P., Warwick, R. S., Snowden, S. L., & Burrows, D. N. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06741.x · Cited by 58
Local ISM 3D distribution and soft X-ray background
Puspitarini, L., Lallement, R., Vergely, J., & Snowden, S. L. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201322942 · Cited by 52
Suzaku Observations of the North Polar Spur: Evidence for Nitrogen Enhancement
Miller, E. D., Tsunemi, H., Bautz, M. W., McCammon, D., Fujimoto, R., Hughes, J. P., Katsuda, S., Kokubun, M., Mitsuda, K., Porter, F. S., et al. (2008) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/60.sp1.s95 · Cited by 50
Banda-Barragán, W., Brüggen, M., Heesen, V., Scannapieco, E., Cottle, J., Federrath, C., & Wagner, A. (2020) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1884 · Cited by 25
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Fujita, Y., Ohira, Y., & Yamazaki, R. (2013) · The Astrophysical Journal · doi:10.1088/2041-8205/775/1/l20 · Cited by 47
“X-ray emission from the high-density gas just behind the shock could have been detected there (Sofue 2000; Bland-Hawthorn & Cohen 2003).”
BackgroundImproved cosmic-ray injection models and the Galactic Center gamma-ray excess
Carlson, E., Linden, T., & Profumo, S. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.94.063504 · Cited by 52
Diffuse X-ray sky in the Galactic center
Koyama, K. (2017) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx084 · Cited by 47
GLOBAL STRUCTURE OF ISOTHERMAL DIFFUSE X-RAY EMISSION ALONG THE FERMI BUBBLES
Kataoka, J., Tahara, M., Totani, T., Sofue, Y., Inoue, Y., Nakashima, S., & Cheung, C. C. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/807/1/77 · Cited by 41
Self-citationMagnetic fields in the solar vicinity and in the Galactic halo
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Panopoulou, G. V., Dickinson, C., Readhead, A. C. S., Pearson, T. J., & Peel, M. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac273f · Cited by 38
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Self-citationThe Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way
Sarkar, K. C. (2024) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-024-00152-1 · Cited by 34
“Several authors proposed that the East-West asymmetry in the NPS could be caused by an East-West density asymmetry, probably due to our Galaxy’s motion ( ∼ 55 km s − 1 ) through the intra-group medium toward the M31 galaxy (Sofue 2000; Mou et al. 2018; Sarkar 2019; Sofue 2019; Mou et al. 2023).”
BackgroundInfluentialTRACING THE MILKY WAY NUCLEAR WIND WITH 21 cm ATOMIC HYDROGEN EMISSION
Lockman, F. J., & McClure-Griffiths, N. M. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/826/2/215 · Cited by 34
On the distance to the North Polar Spur and the local CO-H2factor
Lallement, R., Snowden, S., Kuntz, K. D., Dame, T. M., Koutroumpa, D., Grenier, I., & Casandjian, J. M. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629453 · Cited by 32
“A different interpretation of the NPS enhancement has been defended over the years (Sofue et al. 1974; Sofue 1994, 2000), Article number, page 1 of 15 ar X iv :1 60 9.”
BackgroundThermal and chemical properties of the eROSITA bubbles from Suzaku observations
Gupta, A., Mathur, S., Kingsbury, J., Das, S., & Krongold, Y. (2023) · Nature Astronomy · doi:10.1038/s41550-023-01963-5 · Cited by 31
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Constraints on hot metals in the vicinity of the Galaxy
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The Galactic Central Diffuse X‐Ray Enhancement: A Differential Absorption/Emission Analysis
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Sofue, Y., Kudoh, T., Kawamura, A., Shibata, K., & Fujimoto, M. (2004) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/56.4.633 · Cited by 12
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Supernova-remnant origin of the Galactic-Centre filaments
Sofue, Y. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3137 · Cited by 7
Self-citationKoljonen, K. I. I., Lindseth, S. S., Linares, M., Harding, A. K., & Turchetta, M. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae498 · Cited by 6
Prospects for LOFAR Observations of the Galactic Center
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Borka, V., Milogradov-turin, J., & Urošević, D. (2012) · Cited by 6
Feedback between Sgr A and B: AGN–starburst connection in the galactic centre
Sofue, Y. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2389 · Cited by 6
Self-citationJovanović, V. B., Milogradov‐Turin, J., & Urošević, D. (2008) · Astronomische Nachrichten · doi:10.1002/asna.200610927 · Cited by 4
Cosmic-ray electrons and the magnetic field of the North Polar Spur
Mou, G., Wu, J., & Sofue, Y. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202245401 · Cited by 3
Self-citationHigh Resolution, High Sensitivity Imaging of the Galactic Center at 330 MHz
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Evidence for powerful winds and the associated reverse shock as the origin of the Fermi bubbles
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3D MC. II. X-Ray Echoes Reveal a Clumpy Molecular Cloud in the CMZ
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Prospects for LOFAR Observations of the Galactic Center
Kassim, N. E., Lazio, T. J. W., Nord, M. E., Hyman, S. D., Brogan, C. L., LaRosa, T. N., & Duric, N. (2003) · doi:10.1002/9783527617982.ch10 · Cited by 2
Can the Symmetric Fermi and eROSITA Bubbles Be Produced by Tilted Jets?
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Plasma processes at the scales of galaxies and clusters of galaxiesPreprint
Sharma, P. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1811.12147 · Cited by 2
Loop I/NPS Morphology Predictions in the Ultralong-wavelength Band
Cong, Y., Yue, B., Xu, Y., Deng, F., Zhang, J., & Chen, X. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/adc9a4 · Cited by 1
Growth and merging phenomena of black holes: observational, computational and theoretical efforts
Ter-Kazarian, G. (2021) · Communications of the Byurakan Astrophysical Observatory · doi:10.52526/25792776-2021.68.1-56 · Cited by 1
Multiwavelength Observations of Galactic Winds: Near and Far
Veilleux, S. (2004) · Symposium - International Astronomical Union · doi:10.1017/s0074180900197736
On the Nature of the X-ray Emission from the Galactic Center RegionPreprint
Wang, Q. D., Gotthelf, E. V., & Lang, C. (2002) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0201070
The Fermi Bubbles and Galactic Centre Star Formation
Crocker, R. (2013) · Astrophysics and space science proceedings · doi:10.1007/978-3-642-35410-6_28
Observational aspects of AGN jets at high energy
Kataoka, J. (2014) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921315001775
High Resolution, High Sensitivity Imaging of the Galactic Center at 330 MHz
Nord, M. E., Brogan, C. L., Hyman, S. D., Joseph, T., Lazio, W., Kassim, N. E., LaRosa, T. N., Anantharamaiah, K. R., & Duric, N. (2003) · doi:10.1002/9783527617982.ch2
Kataoka, J. (2020) · Nature Astronomy · doi:10.1038/s41550-020-01269-w
Past activity of Sgr A⋆ is unlikely to affect the local cosmic-ray spectrum up to the TeV regime
Fournier, M., Fensch, J., & Commerçon, B. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450017
Metadata
- Authors
- Sofue, Y.
- Affiliations
- The University of Tokyo (JP)
- Corresponding author
- Sofue, Yoshiaki
- ORCID
- Sofue, Yoshiaki
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2000-09
- Volume
- 540
- Issue
- 1
- Pages
- 224-235
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2050914817
- Cited by
- 102
- References
- 17
- Citations by year
- 2025: 2 · 2024: 8 · 2023: 7 · 2022: 6 · 2021: 5 · 2020: 8 · 2019: 3 · 2018: 7 · 2017: 5 · 2016: 6 · 2015: 7 · 2014: 7 · 2013: 5 · 2012: 3
- FWCI
- 2.68
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- North Polar Spur, shock front, Type II supernovae, radio continuum emission, Galactic halo
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