Hard X-ray emission from a type 2 Seyfert galaxy (NGC 1068)

1988 ◽  
Vol 331 ◽  
pp. 161 ◽  
Author(s):  
Martin Elvis ◽  
A. Lawrence
Keyword(s):  
Seyfert Galaxy ◽  
X Ray ◽  
Ngc 1068

An X-ray image of the Seyfert galaxy NGC 1068

1992 ◽  
Vol 391 ◽  
pp. L75 ◽  
Author(s):  
A. S. Wilson ◽  
M. Elvis ◽  
A. Lawrence ◽  
J. Bland-Hawthorn
Keyword(s):  
Seyfert Galaxy ◽  
X Ray ◽  
Ngc 1068

X-ray evidence of an obscured nucleus in the type 2 Seyfert galaxy Mkn3

Nature ◽  
1990 ◽  
Vol 346 (6284) ◽  
pp. 544-545 ◽  
Author(s):  
H. Awaki ◽  
K. Koyama ◽  
H. Kunieda ◽  
Y. Tawara
Keyword(s):  
Seyfert Galaxy ◽  
X Ray

scholarly journals Tracing the Milky Way’s Vestigial Nuclear Jet

2021 ◽  
Vol 922 (2) ◽  
pp. 254
Author(s):  
Gerald Cecil ◽  
Alexander Y. Wagner ◽  
Joss Bland-Hawthorn ◽  
Geoffrey V. Bicknell ◽  
Dipanjan Mukherjee
Keyword(s):  
Galactic Center ◽  
Galactic Plane ◽  
Hubble Space Telescope ◽  
Seyfert Galaxy ◽  
Radio Continuum ◽  
X Ray ◽  
Multiple Paths ◽  
Ngc 1068 ◽  
Sgr A ◽  
Hydrodynamical Simulations

Abstract MeerKAT radio continuum and XMM-Newton X-ray images have recently revealed a spectacular bipolar channel at the Galactic Center that spans several degrees (∼0.5 kpc). An intermittent jet likely formed this channel and is consistent with earlier evidence of a sustained, Seyfert-level outburst fueled by black hole accretion onto Sgr A* several Myr ago. Therefore, to trace a now weak jet that perhaps penetrated, deflected, and percolated along multiple paths through the interstellar medium, relevant interactions are identified and quantified in archival X-ray images, Hubble Space Telescope Paschen α images and Atacama Large Millimeter/submillimeter Array millimeter-wave spectra, and new SOAR telescope IR spectra. Hydrodynamical simulations are used to show how a nuclear jet can explain these structures and inflate the ROSAT/eROSITA X-ray and Fermi γ-ray bubbles that extend ± 75° from the Galactic plane. Thus, our Galactic outflow has features in common with energetic, jet-driven structures in the prototypical Seyfert galaxy NGC 1068.

scholarly journals The X‐Ray Reflectors in the Nucleus of the Seyfert Galaxy NGC 1068

2002 ◽  
Vol 581 (1) ◽  
pp. 182-196 ◽  
Author(s):  
Edward J. M. Colbert ◽  
Kimberly A. Weaver ◽  
Julian H. Krolik ◽  
John S. Mulchaey ◽  
Richard F. Mushotzky
Keyword(s):  
Seyfert Galaxy ◽  
X Ray ◽  
Ngc 1068

scholarly journals The X-ray nebula around the type 2 Seyfert galaxy NGC 4388

2003 ◽  
Vol 345 (2) ◽  
pp. 369-378 ◽  
Author(s):  
K. Iwasawa ◽  
A. S. Wilson ◽  
A. C. Fabian ◽  
A. J. Young
Keyword(s):  
Seyfert Galaxy ◽  
X Ray

scholarly journals X-ray signatures of the polar dusty gas in AGN

2019 ◽  
Vol 490 (3) ◽  
pp. 4344-4352
Author(s):  
Jiren Liu ◽  
Sebastian F Hönig ◽  
Claudio Ricci ◽  
Stéphane Paltani
Keyword(s):  
Dust Emission ◽  
Galactic Nuclei ◽  
Dusty Gas ◽  
Host Galaxies ◽  
Ionized Gas ◽  
X Ray ◽  
Polar Direction ◽  
Ngc 1068 ◽  
Infrared Interferometry

ABSTRACT Recent mid-infrared interferometry observations of nearby active galactic nuclei (AGN) revealed that a significant part of the dust emission extends in the polar direction, rather than the equatorial torus/disc direction as expected by the traditional unification model. We study the X-ray signatures of this polar dusty gas with ray-tracing simulations. Different from those from the ionized gas, the scattered emission from the polar dusty gas produces self-absorption and neutral-like fluorescence lines, which are potentially a unique probe of the kinematics of the polar dusty gas. The anomalously small Fe Kα/Si Kα ratios of type 2 AGN observed previously can be naturally explained by the polar dusty gas, because the polar emission does not suffer from heavy absorption by the dense equatorial gas. The observed Si Kα lines of the Circinus galaxy and NGC 1068 show blueshifts with respect to the systemic velocities of the host galaxies, consistent with an outflowing scenario of the Si Kα-emitting gas. The 2.5–3 keV image of the Circinus galaxy is elongated along the polar direction, consistent with an origin of the polar gas. These results show that the polar-gas-scattered X-ray emission of type 2 AGN is an ideal objective for future X-ray missions, such as Athena.

Pentacyclic triterpenes, inhibitors of glycogen phosphorylase, as potential drugs for type 2 diabetes: X-ray crystallographic studies

Planta Medica ◽  
2008 ◽  
Vol 74 (09) ◽  
Author(s):  
SE Zographos ◽  
DD Leonidas ◽  
KM Alexacou ◽  
T Gimisis ◽  
JM Hayes ◽  
...  
Keyword(s):  
Type 2 Diabetes ◽  
Glycogen Phosphorylase ◽  
X Ray ◽  
Pentacyclic Triterpenes

scholarly journals The role of AGN activity in the building up of the BCG at z ∼ 1.6

2019 ◽  
Vol 15 (S356) ◽  
pp. 280-284
Author(s):  
Angela Bongiorno ◽  
Andrea Travascio
Keyword(s):  
Galaxy Cluster ◽  
Cluster Galaxy ◽  
X Ray ◽  
Groups Of Galaxies ◽  
Star Forming ◽  
The Core ◽  
The Galaxy ◽  
Multi Wavelength

AbstractXDCPJ0044.0-2033 is one of the most massive galaxy cluster at z ∼1.6, for which a wealth of multi-wavelength photometric and spectroscopic data have been collected during the last years. I have reported on the properties of the galaxy members in the very central region (∼ 70kpc × 70kpc) of the cluster, derived through deep HST photometry, SINFONI and KMOS IFU spectroscopy, together with Chandra X-ray, ALMA and JVLA radio data.In the core of the cluster, we have identified two groups of galaxies (Complex A and Complex B), seven of them confirmed to be cluster members, with signatures of ongoing merging. These galaxies show perturbed morphologies and, three of them show signs of AGN activity. In particular, two of them, located at the center of each complex, have been found to host luminous, obscured and highly accreting AGN (λ = 0.4−0.6) exhibiting broad Hα line. Moreover, a third optically obscured type-2 AGN, has been discovered through BPT diagram in Complex A. The AGN at the center of Complex B is detected in X-ray while the other two, and their companions, are spatially related to radio emission. The three AGN provide one of the closest AGN triple at z > 1 revealed so far with a minimum (maximum) projected distance of 10 kpc (40 kpc). The discovery of multiple AGN activity in a highly star-forming region associated to the crowded core of a galaxy cluster at z ∼ 1.6, suggests that these processes have a key role in shaping the nascent Brightest Cluster Galaxy, observed at the center of local clusters. According to our data, all galaxies in the core of XDCPJ0044.0-2033 could form a BCG of M* ∼ 1012Mȯ hosting a BH of 2 × 108−109Mȯ, in a time scale of the order of 2.5 Gyrs.

scholarly journals Gamma-Ray and Neutrino Signals from Accretion Disk Coronae of Active Galactic Nuclei

Galaxies ◽  
2021 ◽  
Vol 9 (2) ◽  
pp. 36
Author(s):  
Yoshiyuki Inoue ◽  
Dmitry Khangulyan ◽  
Akihiro Doi
Keyword(s):  
Active Galactic Nuclei ◽  
Gamma Ray ◽  
Galactic Nuclei ◽  
High Energy ◽  
Thermal Activity ◽  
X Ray ◽  
Cascade Models ◽  
Coronal Activity ◽  
Ngc 1068 ◽  
High Energy Particles

To explain the X-ray spectra of active galactic nuclei (AGN), non-thermal activity in AGN coronae such as pair cascade models has been extensively discussed in the past literature. Although X-ray and gamma-ray observations in the 1990s disfavored such pair cascade models, recent millimeter-wave observations of nearby Seyferts have established the existence of weak non-thermal coronal activity. In addition, the IceCube collaboration reported NGC 1068, a nearby Seyfert, as the hottest spot in their 10 yr survey. These pieces of evidence are enough to investigate the non-thermal perspective of AGN coronae in depth again. This article summarizes our current observational understanding of AGN coronae and describes how AGN coronae generate high-energy particles. We also provide ways to test the AGN corona model with radio, X-ray, MeV gamma ray, and high-energy neutrino observations.

scholarly journals Ability of radiofrequency echographic multispectrometry to identify osteoporosis status in elderly women with type 2 diabetes

2021 ◽  
Author(s):  
Carla Caffarelli ◽  
Maria Dea Tomai Pitinca ◽  
Antonella Al Refaie ◽  
Elena Ceccarelli ◽  
Stefano Gonnelli
Keyword(s):  
Type 2 Diabetes ◽  
Lumbar Spine ◽  
Elderly Women ◽  
Fragility Fractures ◽  
Dual Energy ◽  
Healthy Controls ◽  
Diagnosis Of Osteoporosis ◽  
X Ray ◽  
The Difference

Abstract Background Patients with type 2 diabetes (T2DM) have an increased or normal BMD; however fragility fractures represent one of the most important complications of T2DM. Aims This study aimed to evaluate whether the use of the Radiofrequency Echographic multi spectrometry (REMS) technique may improve the identification of osteoporosis in T2DM patients. Methods In a cohort of 90 consecutive postmenopausal elderly (70.5 ± 7.6 years) women with T2DM and in 90 healthy controls we measured BMD at the lumbar spine (LS-BMD), at femoral neck (FN-BMD) and total hip (TH-BMD) using a dual-energy X-ray absorptiometry device; moreover, REMS scans were also carried out at the same axial sites. Results DXA measurements were all higher in T2DM than in non-T2DM women; instead, all REMS measurements were lower in T2DM than in non T2DM women. Moreover, the percentage of T2DM women classified as “osteoporotic”, on the basis of BMD by REMS was markedly higher with respect to those classified by DXA (47.0% vs 28.0%, respectively). On the contrary, the percentage of T2DM women classified as osteopenic or normal by DXA was higher with respect to that by REMS (48.8% and 23.2% vs 38.6% and 14.5%, respectively). T2DM women with fragility fractures presented lower values of both BMD-LS by DXA and BMD-LS by REMS with respect to those without fractures; however, the difference was significant only for BMD-LS by REMS (p < 0.05). Conclusions Our data suggest that REMS technology may represent a useful approach to enhance the diagnosis of osteoporosis in patients with T2DM.

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