«PERIASTRON»に関連するポーランド語の本
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1
Atmospheric Dynamics on Strongly Irradiated Jovian Planets - Strona vii
The small points on the orbital diagram show the position of the planet at one-hour intervals; the larger globes (labeled 1 through 4) show the position of the planet at times t = — 19h, Oh, +19h, +38h relative to periastron. The black poles on ...
2
An Astrometric Analysis of Eta Carinae's Eruptive History Using HST ...
Periastron. passage. Given a closest approach of 0.78 A.U., what is the nature of the interaction between the two stars? How large are the tidal forces and is there any mass exchange?
3
Planets Outside the Solar System: Theory and Observations - Strona 99
Plot of the spatial distribution of the periastron of a set of bodies located between 70 and 90 AU and perturbed by a planet on eccentric orbit (Me = 3.10"Me, ep = 0.05, ap = 30 AU). We see that the density of bodies with periastron in the ...
Jean-Marie Mariotti, D.M. Alloin, 2012
4
The Formation and Early Evolution of Stars: From Dust to Stars and ...
periastron separation of the two stars is only 8 stellar radii. [519]. This has a few interesting consequences. One consequence is that as long as the two stars are not near periastron passage, they indeed behave like moderately active CTTS.
5
Astrophysics at Very High Energies: Saas-Fee Advanced Course 40. ...
of the IC flux around the periastron passage. This should lead to an increase of the synchrotron X-radiation which, however, is not observed. Just opposite, the X-ray lightcurve contains a clear minimum at the periastron. It has been claimed ...
Felix Aharonian, Lars Bergström, Charles Dermer, 2013
6
From the Blue Ridge to the Coastal Plain; Field Excursions in the ...
Established by Unger (1856) from the Russchiefer shales in Thuringia, Germany, Periastron was subsequently identified from the New Albany Shale in Indiana and Kentucky and the Lydiennes formation in southern France (Scott and Jeffrey, ...
Martha Cary Eppes, Mervin J. Bartholomew, Geological Society of America, 2012
7
Rotation and Accretion Powered Pulsars - Strona 258
One diagnostic is the behavior of Hα line — the emission site for which is believed to be the Be-star disk — as the neutron star passes around the periastron, accompanied by enhanced X-ray emission due to enhanced accretion. If the disk is ...
8
Proceedings of the Fourth Workshop on Science with the New ...
Time [days relative to periastron I 20 40 60 80 100 PSR B1259–63 • H.E.S.S. data 2004, 2-day average - — Kawachi et al. 2004, misaligned disk (iii) x 0.3 - - - Kirk et al. 1999, dominant adiabatic losses ----- Kirk et al. 1999, dominant radiative ...
Marco Maria Massai, Nicola Omodei, Gloria Spandre, 2007
9
The Twelfth Marcel Grossmann Meeting: On Recent Developments in ...
The HESS observations of this source in 2004, from a few days prior the periastron to several months after the periastron passage, revealed a TeV gamma-ray signal with a high statistical significance. The flux was found to vary significantly on ...
Thibault Damour, Robert Jantzen, Remo Ruffini, 2012
10
Time, Space, Stars and Man: The Story of the Big Bang - Strona 235
Figure 20.6 The modification of an elliptical orbit in a freely-rotating medium showing the effect of forces at periastron and apastron. At periastron the effect is to modify the orbit towards the green form. At apastron the effect is to modify the orbit ...
Michael Mark Woolfson, 2012
用語«PERIASTRON»を含むニュース項目
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Short Story: On Cosmology, by Róisín O'Donell
“Just first year stuff mostly,” I replied, “And the Periastron.” “Shit,” he said, “the Peri-what?” I laughed and took another sip from my glass, “Periastron, it's just . . .”. «Irish Times, 8月 15»
Astro-Challenge: Splitting 44 Boötis
44 Boötis will pass a periastron of just 0.23” from the primary in 2020. Can you split the pair now? How 'bout in 2016 onward? Can you recover the split, post ... «Universe Today, 8月 15»
High-cadence spectra to characterize exoplanets and stars
... star is rapidly accelerating due to the fast approach of its stellar companion τ Boo b to the periastron (the point closest to a star in the path of a body orbiting it). «SPIE Newsroom, 8月 15»
Two Ohio State Grads Want You to Send More Handwritten Notes
Some cards feature quotes, while others feature illustrations or definitions (for example, periastron: when two stars that orbit each other are at their nearest point) ... «Columbus Monthly, 8月 15»
The Universe itself
... story: the orbiting pattern of a binary pulsar (a system of two stars, one of which is a pulsar) exhibits a 'periastron shift' analogous to Mercury's perihelion shift. «Nature.com, 7月 15»
N.J. student eliminated in semifinals of National Spelling Bee
She survived the first semifinal round by correctly spelling periastron, the point in an orbit where a body is closest to the star it is orbiting. Wang, who finished ... «NJ.com, 5月 15»
Eta Carinae's Throbbing X-ray Pulse
But when closest to each other, at periastron, the two flows collide violently, creating a shock boundary that heats the gas to tens of millions of degrees — hot ... «Sky & Telescope, 1月 15»
Video: Superstar Eta Carinae
At their closest approach, or periastron, the stars are only 140 million miles (225 million kilometers) apart, or about the average distance between Mars and the ... «EarthSky, 1月 15»
Massive Eta Carinae's Great Eruptions Baffle Astronomers
At closest approach, or periastron, the stars are 140 million miles (225 million kilometers) apart, or about the average distance between Mars and the sun. «The Daily Galaxy, 1月 15»
Image of the Day --The Eta Carinae Superstar: Site of the "Great …
However, when the two stars are at their closest during their orbit (a point that astronomers call “periastron”), the X-ray emission dips unexpectedly. «The Daily Galaxy, 9月 14»
