Zobrazeno 1 - 10
of 14
pro vyhledávání: '"E. K. Verolme"'
Publikováno v:
Journal of Loss Prevention in the Process Industries, 51, 54-64
There is limited knowledge on deriving the strength of an explosion based on the observed explosion effects. Existing methods are based primarily on the effects of blast overpressure on surrounding structures. Window breakage and structural damage ar
Autor:
E. K. Verolme, Arjan Mieremet
Publikováno v:
Forensic science international. 278
Forensic investigations are primarily meant to obtain objective answers that can be used for criminal prosecution. Accident analyses are usually performed to learn from incidents and to prevent similar events from occurring in the future. Although th
Autor:
G. D. Illingworth, R. P. van der Marel, P. T. de Zeeuw, C. M. Carollo, M. Franx, M. Cappellari, E. K. Verolme, G. A. Verdoes Kleijn
The E3 giant elliptical galaxy IC1459 is the prototypical galaxy with a fast counterrotating stellar core. We obtained one HST/STIS long-slit spectrum along the major axis of this galaxy and CTIO spectra along five position angles. We present self-co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd273619fdd9b22f02c22e3b4ef402e2
https://ora.ox.ac.uk/objects/uuid:b5f3dbdc-281b-46c5-aa87-cbb8fdea83d3
https://ora.ox.ac.uk/objects/uuid:b5f3dbdc-281b-46c5-aa87-cbb8fdea83d3
Autor:
E. K. Verolme, Harald Kuntschner, G. Monnet, C. Marcella Carollo, P. Tim de Zeeuw, Bryan W. Miller, Reynier Peletier, Y. Copin, Roger L. Davies, Martin Bureau, Eric Emsellem, R. Bacon
We report the first wide-field mapping of the kinematics and stellar populations in the E3 galaxy NGC 4365. The velocity maps extend previous long-slit work. They show two independent kinematic subsystems: the central 300 x 700 pc rotates about the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a05098ad7bc2275b66eec25d987f869
https://ora.ox.ac.uk/objects/uuid:6e7dd72d-296f-4656-8b00-596c7f71daac
https://ora.ox.ac.uk/objects/uuid:6e7dd72d-296f-4656-8b00-596c7f71daac
Autor:
R. P. van der Marel, B. M. Miller, Y. Copin, P. T. de Zeeuw, E. K. Verolme, Michele Cappellari, Roland Bacon, Roger L. Davies, Martin Bureau
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2002, 335, pp.517-525. ⟨10.1046/j.1365-8711.2002.05664.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2002, 335, pp.517-525. ⟨10.1046/j.1365-8711.2002.05664.x⟩
We present dynamical models of the nearby compact elliptical galaxy M32, using high quality kinematical measurements, obtained with the integral-field spectrograph SAURON mounted on the William Herschel Telescope on La Palma. We also include STIS dat
Autor:
E. K. Verolme, P. T. de Zeeuw
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 331:959-968
We describe a practical method for constructing axisymmetric two-integral galaxy models (with distribution functions of the form f(E,L_z), in which E is the orbital energy, and L_z is the vertical component of the angular momentum), based on Schwarzs
Autor:
Jeremy R. Allington-Smith, Y. Copin, C.M. Carollo, Roland Bacon, P. T. de Zeeuw, Reynier Peletier, Martin Bureau, Eric Emsellem, B. W. Miller, Roger L. Davies, E. K. Verolme, G. Monnet
Publikováno v:
New Astronomy Reviews. 45:83-86
We present the first results from a new and unique integral-field spectrograph, SAURON, for the 4.2-m William Herschel Telescope on La Palma. Based upon the TIGER concept, SAURON uses a lens array to obtain two-dimensional spectroscopy with complete
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 385(2)
We present a flexible and efficient method to construct triaxial dynamical models of galaxies with a central black hole, using Schwarzschild's orbital superposition approach. Our method is general and can deal with realistic luminosity distributions,
Publikováno v:
International Journal of Impact Engineering, 2, 35, 109-118
A deterministic model has been developed that describes the throw of debris or fragments from a source with an arbitrary geometry and for arbitrary initial conditions. The initial conditions are defined by the distributions of mass, launch velocity a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a1b56371002dda3d9568813e38fb7730
http://resolver.tudelft.nl/uuid:f7bf17f2-7cf9-4229-ba2f-b2dc0ad24729
http://resolver.tudelft.nl/uuid:f7bf17f2-7cf9-4229-ba2f-b2dc0ad24729
We determine the dynamical distance D, inclination i, mass-to-light ratio M/L and the intrinsic orbital structure of the globular cluster omega Cen, by fitting axisymmetric dynamical models to the ground-based proper motions of van Leeuwen et al. and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7622a101106954f7d5ebffb7f5ba02c6