24 research outputs found
Follow-up observations of pulsating subdwarf B stars: Multisite campaigns on PG 1618+563B and PG 0048+091
We present follow-up observations of pulsating subdwarf B (sdB) stars as part
of our efforts to resolve the pulsation spectra for use in asteroseismological
analyses. This paper reports on multisite campaigns of the pulsating sdB stars
PG 1618+563B and PG 0048+091. Data were obtained from observatories placed
around the globe for coverage from all longitudes. For PG 1618+563B, our
five-site campaign uncovered a dichotomy of pulsation states: Early during the
campaign the amplitudes and phases (and perhaps frequencies) were quite
variable while data obtained late in the campaign were able to fully resolve
five stable pulsation frequencies. For PG 0048+091, our five-site campaign
uncovered a plethora of frequencies with short pulsation lifetimes. We find
them to have observed properties consistent with stochastically excited
oscillations, an unexpected result for subdwarf B stars. We discuss our
findings and their impact on subdwarf B asteroseismology.Comment: 50 pages including 17 figures and 10 tables. Accepted for publication
in the Astrophysical Journa
Towards ensemble asteroseismology of the young open clusters Chi Persei and NGC 6910
As a result of the variability survey in Chi Persei and NGC6910, the number
of Beta Cep stars that are members of these two open clusters is increased to
twenty stars, nine in NGC6910 and eleven in Chi Persei. We compare pulsational
properties, in particular the frequency spectra, of Beta Cep stars in both
clusters and explain the differences in terms of the global parameters of the
clusters. We also indicate that the more complicated pattern of the variability
among B type stars in Chi Persei is very likely caused by higher rotational
velocities of stars in this cluster. We conclude that the sample of pulsating
stars in the two open clusters constitutes a very good starting point for the
ensemble asteroseismology of Beta Cep-type stars and maybe also for other
B-type pulsators.Comment: 4 pages, Astronomische Nachrichten, HELAS IV Conference, Arecife,
Lanzarote, Feb 2010, submitte
Photometric multi-site campaign on the open cluster NGC 884 I. Detection of the variable stars
CONTEXT: Recent progress in the seismic interpretation of field beta Cep
stars has resulted in improvements of the physics in the stellar structure and
evolution models of massive stars. Further asteroseismic constraints can be
obtained from studying ensembles of stars in a young open cluster, which all
have similar age, distance and chemical composition.
AIMS: To improve our comprehension of the beta Cep stars, we studied the
young open cluster NGC 884 to discover new B-type pulsators, besides the two
known beta Cep stars, and other variable stars.
METHODS: An extensive multi-site campaign was set up to gather accurate CCD
photometry time series in four filters (U, B, V, I) of a field of NGC884.
Fifteen different instruments collected almost 77500 CCD images in 1286 hours.
The images were calibrated and reduced to transform the CCD frames into
interpretable differential light curves. Various variability indicators and
frequency analyses were applied to detect variable stars in the field. Absolute
photometry was taken to deduce some general cluster and stellar properties.
RESULTS: We achieved an accuracy for the brightest stars of 5.7 mmag in V,
6.9 mmag in B, 5.0 mmag in I and 5.3 mmag in U. The noise level in the
amplitude spectra is 50 micromag in the V band. Our campaign confirms the
previously known pulsators, and we report more than one hundred new multi- and
mono-periodic B-, A- and F-type stars. Their interpretation in terms of
classical instability domains is not straightforward, pointing to imperfections
in theoretical instability computations. In addition, we have discovered six
new eclipsing binaries and four candidates as well as other irregular variable
stars in the observed field.Comment: Accepted for publication in Astronomy and Astrophysics, 21 pages, 14
figures, 4 tables. The full appendix is available at
http://www.ster.kuleuven.be/~sophies/Appendix.pdf (74 MB, 169 pages, 343
figures, 1 table
Death anxiety resilience; a mixed methods investigation
Research was conducted examining how death anxiety influenced PTSD and mental health among people who have experienced a life-threatening event. This study was conducted using undergraduate university students in Lithuania. The study used a mixed-method design and in phase 1, participants (N = 97) completed self-report questionnaires that gathered information on demographics, death anxiety, trauma and well-being. Data indicated a significant correlation between death anxiety and PTSD, but not psychiatric co-morbidity. Phase 2 attempted to further explore the phenomenological experience of participants with full PTSD, and 6 semi-structured interviews were conducted. IPA analysis found three major themes in response to the life-threatening event; self-efficacy, religious coping and existential attitude. Overall these coping mechanisms allowed participants to develop resilience against the effects of death anxiety and minimize its negative impact on mental health
The ongoing 2005 -- 2006 campaign on beta Cephei stars in NGC 6910 and chi Persei (NGC 884)
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The ongoing 2005 -- 2006 campaign on beta Cephei stars in NGC 6910 and chi Persei (NGC 884)
Not Availabl
The ongoing 2005 -- 2006 campaign on beta Cephei stars in NGC 6910 and chi Persei (NGC 884)
International audienc