Bibcode
Middleton, M. J.; Casella, P.; Gandhi, P.; Bozzo, E.; Anderson, G.; Degenaar, N.; Donnarumma, I.; Israel, G.; Knigge, C.; Lohfink, A.; Markoff, S.; Marsh, T.; Rea, N.; Tingay, S.; Wiersema, K.; Altamirano, D.; Bhattacharya, D.; Brandt, W. N.; Carey, S.; Charles, P.; Díaz Trigo, M.; Done, C.; Kotze, M.; Eikenberry, S.; Fender, R.; Ferruit, P.; Fürst, F.; Greiner, J.; Ingram, A.; Heil, L.; Jonker, P.; Komossa, S.; Leibundgut, B.; Maccarone, T.; Malzac, J.; McBride, V.; Miller-Jones, J.; Page, M.; Rossi, E. M.; Russell, D. M.; Shahbaz, T.; Sivakoff, G. R.; Tanaka, M.; Thompson, D. J.; Uemura, M.; Uttley, P.; van Moorsel, G.; van Doesburgh, M.; Warner, B.; Wilkes, B.; Wilms, J.; Woudt, P.
Bibliographical reference
New Astronomy Reviews, Volume 79, p. 26-48.
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11
2017
Journal
Citations
19
Refereed citations
12
Description
Whilst astronomy as a science is historically founded on observations at
optical wavelengths, studying the Universe in other bands has yielded
remarkable discoveries, from pulsars in the radio, signatures of the Big
Bang at submm wavelengths, through to high energy emission from
accreting, gravitationally-compact objects and the discovery of
gamma-ray bursts. Unsurprisingly, the result of combining multiple
wavebands leads to an enormous increase in diagnostic power, but
powerful insights can be lost when the sources studied vary on
timescales shorter than the temporal separation between observations in
different bands. In July 2015, the workshop ;Paving the way to
simultaneous multi-wavelength astronomy; was held as a concerted effort
to address this at the Lorentz Center, Leiden. It was attended by 50
astronomers from diverse fields as well as the directors and staff of
observatories and spaced-based missions. This community white paper has
been written with the goal of disseminating the findings of that
workshop by providing a concise review of the field of multi-wavelength
astronomy covering a wide range of important source classes, the
problems associated with their study and the solutions we believe need
to be implemented for the future of observational astronomy. We hope
that this paper will both stimulate further discussion and raise overall
awareness within the community of the issues faced in a developing,
important field.
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Black holes, neutron stars, white dwarfs and their local environment
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only confirmation of the existence of stellar mass black holes via dynamical mass measurements, but also the best opportunity for probing high-gravity environments and the physics of accretion; the most
Montserrat
Armas Padilla