Article
Astronomy & Astrophysics
K. Iwasawa, C. Norman, R. Gilli, P. Gandhi, M. A. Perez-Torres
Summary: We present a spatially resolved, X-ray spectroscopic study of the diffuse emission found in the central part of nearby starburst galaxy M 82, providing new details and important conclusions about the nature and origin of the hot gas and its impact on the interstellar medium. Using archival data from the Chandra X-ray Observatory, we find that the Fe XXV emission is enhanced only in a limited area close to the starburst disc, indicating the presence of non-thermal emission due to inverse Compton scattering. Our study also suggests that the majority of the 4-8 keV luminosity originates from inverse Compton emission, while the metal-rich hot gas makes a minor contribution to the continuum but accounts for the observed Fe XXV line. Furthermore, we find that the hot gas emerges from the circumnuclear starburst ring and fills the galactic chimneys identified as mid-infrared and radio emission voids, suggesting that supernova energy in the starburst site is transported to the halo through these chimneys.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Souradeep Bhattacharya, Magda Arnaboldi, Francois Hammer, Yanbin Yang, Ortwin Gerhard, Nelson Caldwell, Kenneth C. Freeman
Summary: By measuring the line-of-sight velocities of planetary nebulae, it is found that there are multiple substructures in the inner halo of M 31, such as G1-Clump, NE-, and W-shelves, and the Giant Stream. The formation of these substructures is consistent with a major merger event, indicating a recent significant merger in M 31.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
K. Iwasawa
Summary: Researchers searched for X-ray supernova remnants (SNRs) in the starburst region of M82 using data from the Chandra X-ray Observatory. They identified six (possibly seven) candidates with characteristic features of youth, some of which have radio counterparts. An estimate of supernova rate was made based on the luminosity of the selected SNRs, showing agreement with previously estimated rates. The selected SNRs contribute significantly to the total Fe xxv luminosity in M82 and have implications for starburst winds and Fe xxv emission in more luminous starburst galaxies.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
S. Hancock, A. J. Young, P. Chainakun
Summary: We analyzed a sample of 20 active galactic nuclei (AGNs) using the XMM-Newton archive, focusing on the reverberation signatures caused by X-ray reflection from the accretion disc. Our study found that the black hole mass and time lag exhibit a well-recovered scaling relationship, and the continuum flux is strongly coupled to the disc reflection flux. Additionally, we observed a correlation between the reflection fraction and the power-law photon index, suggesting a possible link to the dynamics of the emitting region.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Souradeep Bhattacharya, Magda Arnaboldi, Ortwin Gerhard, Alan McConnachie, Nelson Caldwell, Johanna Hartke, Kenneth C. Freeman
Summary: The study aims to determine the origin of substructures in the M 31 galaxy by examining the properties of planetary nebulae in its inner halo. Results suggest that some substructures are likely remnants of accreted satellites while others are linked to the pre-merger disc with contributions from younger stars. Additionally, the faint-end of the planetary nebula luminosity function is found to be populated by those evolved from older stars.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
M. S. Mirakhor, S. A. Walker
Summary: By utilizing XMM-Newton observations, the formation scenarios and AGN occupation fraction of ultradiffuse galaxies (UDGs) in the nearby Coma cluster were probed. The measurements suggest that UDGs are puffed-up dwarf galaxies and the AGN occupation fraction of UDGs was determined by cross-correlating their positions with detected point sources in Coma.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Arghajit Jana, Neeraj Kumari, Prantik Nandi, Sachindra Naik, Arka Chatterjee, Gaurava K. Jaisawal, Kimitake Hayasaki, Claudio Ricci
Summary: The study on the changing-look active galactic nucleus NGC 1566 during its outburst in June 2018 revealed a significant increase in X-ray intensity. Analysis of the X-ray data and modeling showed a strong soft X-ray excess during the outburst, potentially originating from the warm Comptonizing region in the inner accretion disc. The sudden rise in luminosity observed is likely caused by an increase in the accretion rate.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Prantik Nandi, Arka Chatterjee, Sandip K. Chakrabarti, Broja G. Dutta
Summary: The study analyzed the long-term X-ray spectral and temporal properties of a bare-type AGN, revealing that spectral variations can be explained by changes in accretion dynamics. The correlation between X-ray time delays and soft-excess suggests a common physical process.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Roberto Soria, Mari Kolehmainen, Alister W. Graham, Douglas A. Swartz, Mihoko Yukita, Christian Motch, Thomas H. Jarrett, James C. A. Miller-Jones, Richard M. Plotkin, Thomas J. Maccarone, Laura Ferrarese, Alexander Guest, Ariane Lancon
Summary: In this study, we analyze the population of ultraluminous X-ray sources (ULXs) in late-type galaxies in the Virgo cluster. We find that the ULX luminosity function is related to the mass and star formation rate of the galaxies, and we tentatively identify the most luminous X-ray source as a recent supernova or its remnant.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
K. Kouroumpatzakis, A. Zezas, A. Wolter, A. Fruscione, K. Anastasopoulou, A. Prestwich
Summary: This systematic study of the metallicity variations within the collisional ring galaxy NGC922 reveals a difference in metallicity between star-forming regions in the bulge and the ring. The study also shows an anticorrelation between X-ray luminosity and metallicity of the sub-galactic regions of NGC922.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
M. S. Mirakhor, S. A. Walker, J. Bagchi, A. C. Fabian, A. J. Barth, F. Combes, P. Dabhade, L. C. Ho, M. B. Pandge
Summary: In this study, a deep XMM-Newton observation of the spiral galaxy 2MASX J23453268-0449256 revealed the presence of diffuse X-ray emission from the hot gaseous halo, corresponding to 35% of the virial radius and constituting approximately 65% of the galaxy's total baryon mass content. The estimated energy densities of electrons and magnetic field in the radio lobes associated with the galaxy suggest an electron-dominated composition, with a factor of 10-200 depending on the lower cut-off energy of the electron spectrum.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
S. Allak, A. Akyuz, I. Akkaya Oralhan, S. Avdan, N. Aksaker, A. Vinokurov, F. Soydugan, E. Sonbas, K. S. Dhuga
Summary: In this study, we analyzed the ULX-4 transient source in the M51 galaxy using temporal and spectral analysis techniques. The X-ray flux of the source showed significant variation within a month, but no short-term variability was observed within the time intervals of 100-2000 s. We found evidence of a bi-modality feature in the flux distribution of ULX-4. Based on optical counterparts identified using Hubble Space Telescope data, the spectral type of ULX-4 was determined to be B-type stars. One of the counterparts exhibited a weak periodicity, which could be associated with orbital motion of a red supergiant donor or interactions with a circumstellar disc in the case of a Be/X star.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
H. Avdan, E. Sonbas, K. S. Dhuga, A. Vinokurov, E. Goegues, S. Avdan, Y. N. Solovyeva, A. E. Kostenkov, E. S. Shablovinskaya, D. Goktas
Summary: Archival data from XMM-Newton, Chandra, and Hubble Space Telescope were used to study the X-ray and optical properties of two ultraluminous X-ray sources in NGC 4536. Improved astrometry between Chandra and HST allowed for the detection of optical counterparts for both sources. Ground-based optical spectra were obtained with the BTA Telescope to complement the archival data.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
N. Sahakyan
Summary: The long-term multiwavelength study of the powerful flat spectrum radio quasar 3C 454.3 using Fermi LAT and Swift XRT/UVOT data revealed major flares in the gamma-ray, X-ray, and optical/UV bands. Modelling of 362 high-quality spectral energy distributions showed that emission during flares likely originated in a faster moving region within the jet of 3C 454.3. The study provides insights into the underlying emission mechanisms and evolution of the physical parameters of the jet over time.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
N. Sahakyan, P. Giommi
Summary: We present the results of a comprehensive analysis of the observations of the BL Lac object prototype BL Lacertae, covering a period of almost 13 years. The source exhibits strong variability in emission at all frequencies, with frequent spectral changes. Notably, several prominent gamma-ray flares, including one reaching a flux of (4.39 +/- 1.01) x 10(-6) photon cm(-2) s(-1), have been detected. The X-ray spectral variability during the brightest flare indicates a shift of the synchrotron peak to a higher frequency range. We systematically investigate the multiwavelength emission of BL Lacertae using leptonic models and find that the majority of the observed spectral energy distributions can be explained with a one-zone model. However, a two-zone leptonic scenario is required for a smaller subset of SEDs with soft and bright X-ray spectra and high energy gamma-ray observations. The HBL behavior observed during the brightest X-ray flare suggests the presence of a second emission zone beyond the broad-line region.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)