33 research outputs found
X-ray variability in a complete sample of Soft X-ray selected AGN
We present ROSAT All-Sky Survey and ROSAT pointed observations (PSPC and HRI)
of a complete sample of 113 bright soft X-ray AGN selected from the ROSAT
Bright Source Catalog. We compare these observations in order to search for
extreme cases of flux and spectral X-ray variability - X-ray transient AGN.
Three definite transients and one transient candidate are found.
The other sources show amplitude variations typically by factors of 2-3 on
timescales of years. We found that the variability strength on timescales of
days is a function of the steepness of the X-ray spectrum: steeper X-ray
objects show stronger variability than flat X-ray spectrum sources. We also
present new HRI measurements of our extreme X-ray transients IC 3599 and
WPVS007. We discuss possible models to explain the X-ray transience and the
variabilities observed in the non-transient sources.Comment: 17 pages (including 7 Figures), accepted for in A&A (main journal),
also available at http://www.xray.mpe.mpg.de/~dgrupe/research/refereed.htm
X-ray Absorption and Reflection in Active Galactic Nuclei
X-ray spectroscopy offers an opportunity to study the complex mixture of
emitting and absorbing components in the circumnuclear regions of active
galactic nuclei, and to learn about the accretion process that fuels AGN and
the feedback of material to their host galaxies. We describe the spectral
signatures that may be studied and review the X-ray spectra and spectral
variability of active galaxies, concentrating on progress from recent Chandra,
XMM-Newton and Suzaku data for local type 1 AGN. We describe the evidence for
absorption covering a wide range of column densities, ionization and dynamics,
and discuss the growing evidence for partial-covering absorption from data at
energies > 10 keV. Such absorption can also explain the observed X-ray spectral
curvature and variability in AGN at lower energies and is likely an important
factor in shaping the observed properties of this class of source.
Consideration of self-consistent models for local AGN indicates that X-ray
spectra likely comprise a combination of absorption and reflection effects from
material originating within a few light days of the black hole as well as on
larger scales. It is likely that AGN X-ray spectra may be strongly affected by
the presence of disk-wind outflows that are expected in systems with high
accretion rates, and we describe models that attempt to predict the effects of
radiative transfer through such winds, and discuss the prospects for new data
to test and address these ideas.Comment: Accepted for publication in the Astronomy and Astrophysics Review. 58
pages, 9 figures. V2 has fixed an error in footnote
The tidal disruption event AT2017eqx:spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow
We present and analyse a new tidal disruption event (TDE), AT2017eqx at
redshift z=0.1089, discovered by Pan-STARRS and ATLAS. The position of the
transient is consistent with the nucleus of its host galaxy; it peaks at a
luminosity of erg s; and the spectrum shows a
persistent blackbody temperature K with broad H I and He II
emission. The lines are initially centered at zero velocity, but by 100 days
the H I lines disappear while the He II develops a blueshift of
km s. Both the early- and late-time morphologies have been seen in other
TDEs, but the complete transition between them is unprecedented. The evolution
can be explained by combining an extended atmosphere, undergoing slow
contraction, with a wind in the polar direction becoming visible at late times.
Our observations confirm that a lack of hydrogen a TDE spectrum does not
indicate a stripped star, while the proposed model implies that much of the
diversity in TDEs may be due to the observer viewing angle. Modelling the light
curve suggests AT2017eqx resulted from the complete disruption of a solar-mass
star by a black hole of . The host is another quiescent,
Balmer-strong galaxy, though fainter and less centrally concentrated than most
TDE hosts. Radio limits rule out a relativistic jet, while X-ray limits at 500
days are among the deepest for a TDE at this phase.Comment: Updated to match published versio
New insights into the synergism of nucleoside analogs with radiotherapy
Nucleoside analogs have been frequently used in combination with radiotherapy in the clinical setting, as it has long been understood that inhibition of DNA repair pathways is an important means by which many nucleoside analogs synergize. Recent advances in our understanding of the structure and function of deoxycytidine kinase (dCK), a critical enzyme required for the anti-tumor activity for many nucleoside analogs, have clarified the mechanistic role this kinase plays in chemo- and radio-sensitization. A heretofore unrecognized role of dCK in the DNA damage response and cell cycle machinery has helped explain the synergistic effect of these agents with radiotherapy. Since most currently employed nucleoside analogs are primarily activated by dCK, these findings lend fresh impetus to efforts focused on profiling and modulating dCK expression and activity in tumors. In this review we will briefly review the pharmacology and biochemistry of the major nucleoside analogs in clinical use that are activated by dCK. This will be followed by discussions of recent advances in our understanding of dCK activation via post-translational modifications in response to radiation and current strategies aimed at enhancing this activity in cancer cells
Multi-messenger observations of a binary neutron star merger
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transientâs position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta
Multi-messenger Observations of a Binary Neutron Star Merger
On 2017 August 17 a binary neutron star coalescence candidate (later
designated GW170817) with merger time 12:41:04 UTC was observed through
gravitational waves by the Advanced LIGO and Advanced Virgo detectors.
The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray
burst (GRB 170817A) with a time delay of ⌠1.7 {{s}} with respect to
the merger time. From the gravitational-wave signal, the source was
initially localized to a sky region of 31 deg2 at a
luminosity distance of {40}-8+8 Mpc and with
component masses consistent with neutron stars. The component masses
were later measured to be in the range 0.86 to 2.26 {M}ÈŻ
. An extensive observing campaign was launched across the
electromagnetic spectrum leading to the discovery of a bright optical
transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC
4993 (at ⌠40 {{Mpc}}) less than 11 hours after the merger by the
One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The
optical transient was independently detected by multiple teams within an
hour. Subsequent observations targeted the object and its environment.
Early ultraviolet observations revealed a blue transient that faded
within 48 hours. Optical and infrared observations showed a redward
evolution over âŒ10 days. Following early non-detections, X-ray and
radio emission were discovered at the transientâs position ⌠9
and ⌠16 days, respectively, after the merger. Both the X-ray and
radio emission likely arise from a physical process that is distinct
from the one that generates the UV/optical/near-infrared emission. No
ultra-high-energy gamma-rays and no neutrino candidates consistent with
the source were found in follow-up searches. These observations support
the hypothesis that GW170817 was produced by the merger of two neutron
stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and
a kilonova/macronova powered by the radioactive decay of r-process
nuclei synthesized in the ejecta.</p
2-Chlorodeoxyadenosine to Treat Refractory Histiocytosis X
To the Editor:
Treatment of histiocytosis X is palliative at best. It includes corticosteroids, alkylating agents, antimetabolites, vinca alkaloids, and irradiation
1
. Since 2-chlorodeoxyadenosine, a purine substrate analogue active against lymphoid cancers,
2
is toxic to monocytes in vitro,
3
and since tissue histiocytes are derived from circulating monocytes as they move from the intravascular space to soft tissues, we administered 2-chlorodeoxyadenosine to a patient with histiocytosis X.
A 33-year-old woman had presented at the age of 15 years with polyuria and polydipsia due to diabetes insipidus. Two years later vesiculopustular lesions developed on her gingiva, scalp, and vagina that were histologically . .Â