CĂRȚI ÎN ENGLEZĂ ÎN LEGĂTURĂ CU «ISOPHOTAL»
Descoperă întrebuințarea
isophotal în următoarea selecție bibliografică. Cărți în legătură cu
isophotal și extrase din aceasta pentru a furniza contextul de întrebuințare al acestuia în literatura Engleză.
1
Astronomical Photometry: A Guide
Consequently, Eq. (1.39) cannot be valid. It is, of course, possible to find, for
every observation, a particular wavelength where monochromatic measurements
would reproduce the heterochromatic data. The isophotal wavelength X\ is
precisely ...
C. Sterken, J. Manfroid, 1992
2
Galaxies: Interactions and Induced Star Formation: Saas-Fee ...
Fourth, in most E galaxies the isophotal ellipticity changes as a function of radius.
It can increase, decrease, or vary irregularly with increasing radius (Liller 1961;
King 1978; Jedrzejewski 1987a; Franx et al. 1989a; and many since).
R. C. Kennicutt, F. Schweizer, J.E. Barnes, 1998
2.3.6 Surface brightness and isophotal radii To this point we have been
concerned with total brightnesses and luminosities. Galaxies, unlike most stars,
are resolved objects, so that in addition to measuring the total radiative flux from
a galaxy, ...
James Binney, Michael Merrifield, 1998
4
The High Altitude Observatory
Isophotal Contour Densitometer
Because of the limitations for this work of other contouring methods the staff of the High Altitude Observatory has sought to develop a new type photometer capable of analyzing films from motion picture sequences fast enough for the problem ...
Fred E. Fowler, Donald S. Johnson, Donald E. Billings, 1952
5
Morphological and Physical Classification of Galaxies: ...
THE ORIGIN OF STRONG ISOPHOTAL TWISTS IN ELLIPTICAL GALAXIES1 J.-L.
Nieto and Ch. Lagoute Observatoire Midi-Pyrenees Toulouse, France Strong
isophotal twists in elliptical galaxies have been one of the major clues to our ...
Osservatorio astronomico di Capodimonte. International Workshop, G. Longo, Massimo Capaccioli, 1992
6
Studies of the Structure and Evolution of the Intracluster ...
0 0.2 0.4 0.6 0.8 1 Figure 4.13 — Constraints on Om and £l\ from fitting the
angular diameter distances determined from isophotal sizes. The thick and thin
contours mark the boundaries of the 1 and 2a confidence regions, respectively.
Timothy Brian O'Hara, 2007
7
Formation and Evolution of Galaxy Bulges (IAU S245)
Star. formation. history. and. isophotal. shapes. of. fossil. central. galaxies. Habib
G. Khosroshahi1 f and Louisa A. Nolan1 'School of Physics and Astronomy,
University of Birmingham, B15 2TT, UK email: ...
International Astronomical Union. Symposium, Martin Bureau, E. Athanassoula, 2008
8
Chaos in Astronomy: Conference 2007
We show that disc mergers alone are unlikely to form a boxy-discy dichotomy in
isophotal shape, because of the survival of disc-like orbits even in violent
mergers. The shape of the different orbit families can vary strongly, depending on
how ...
G. Contopoulos, P. A. Patsis, 2009
9
To Measure the Sky: An Introduction to Observational Astronomy
10.5 (a) Effective wavelengths for two different sources in the same band. The
solid curves apply to a hot source, and the dotted curves apply to a cool source
with the same magnitude in the band. (b) Definition of the isophotal wavelength:
the ...
Frederick R. Chromey, 2010
10
The Deep Universe: Saas-Fee Advanced Course 23. Lecture ...
Swiss Society for Astrophysics and Astronomy A.R. Sandage R.G. Kron, M.S.
Longair, Bruno Binggeli, Roland Buser. due to the decrease in the surface
brightness by the (1 + z)4 factor. The ratio of metric to isophotal diameter as a
function of ...
A.R. Sandage, R.G. Kron, M.S. Longair, 1995
ȘTIRI NOI CARE INCLUD TERMENUL «ISOPHOTAL»
Află ce ziare naționale și internaționale au scris despre și cum este întrebuințat termenul
isophotal în contextul următoarelor știri.
A runaway collision in a young star cluster as the origin of the …
19) into account, that within the observed isophotal magnitude B25 approximately 16'' ( approx 5.6 kpc) and adopting M/LB proportional to ... «Nature.com, Nov 07»
