与 «ECLIPSING VARIABLE»相关的英语书籍
在以下的参考文献中发现
eclipsing variable的用法。与
eclipsing variable相关的书籍以及同一来源的简短摘要提供其在 英语文献中的使用情境。
1
Understanding
Variable Stars
Bright and/or interesting eclipsing variable stars more exciting. The radiation from
one component, usually the hotter one, may also irradiate the other component,
producing an observable effect in the light curve. Nevertheless, professional ...
2
Eclipsing Binary Stars: Modeling and Analysis: Modeling and ...
I, ApJ 35, 315–340 Russell, H. N.: 1912b, On the Determination of the Orbital
Elements of Eclipsing Variable Stars. II, ApJ 36, 54–74 Russell, H. N. & Merrill,
J. E.: 1952, The Determination of the Elements of Eclipsing Binary Stars,
Princeton.
Josef Kallrath, Eugene F. Milone,
2009
3
Observing
Variable Stars
Table 7.1. Eclipsing variable stars arranged in alphabetical order by designation
Variable type Algol type P Lyr type Planetary eclipsing type W UMa type RS
Canum Venaticorum Designation (and subclasses) EA Algol-type eclipsing
system ...
4
Observing
Variable Stars, Novae and Supernovae
... 156, 181, 180-183, 186, 213 eclipsing dwarf novae 180-183 eclipsing variable
stars see eclipsing binary systems Eddington, Sir Arthur 126, 127, 128-129
effective temperature 112 ELL stars see rotating variable stars electron
degeneracy ...
5
Variable Stars and Stellar Evolution
The eclipsing variable V65 is at quite a large angular distance, 16'1, from the
cluster center; yet close to its position are the RR Lyrae stars V 55, V 64 and the
red variable V 68. From a preliminary analysis of the photometric measurements
of V ...
V.E. Sherwood, L. PLAUT (Ed),
1975
6
Light Curves of
Variable Stars: A Pictorial Atlas
The prototype of the RS type is RS Canum Venaticorum, which was discovered
as an eclipsing variable in 1914 by W. Ceraski. The starspot wave between
eclipses was seen in the 1920-1922 light curve obtained by Bancroft Walker
Sitterly ...
C. Sterken, C. Jaschek,
2005
7
An Introduction to Close Binary Stars
The classification scheme that was adopted and continues to be used now for the
great majority of eclipsing variables is the following: EA An eclipsing variable of
the Algol type, meaning that its light curve has similarities to that of Algol itself, ...
8
Astronomy and Cosmogony
The light received from such a system accordingly varies, and the system is
described as an "eclipsing variable," -or an "eclipsing binary." It will be
understood that physically an eclipsing binary is precisely similar to a non-
eclipsing binary ; thn ...
9
The Study of
Variable Stars Using Small Telescopes
... see eclipsing variable stars Eclipsing variable stars, 14-16, 18, 21- 23, 27, 35-
39, 64-65, 71, 73, 83, 94, 177, 239-240, 259 evolution, 65 light curve, 38 method
of observing, 18 Eruptive variable stars, 13-14, 25-26; Eruptive variable stars, ...
John R. Percy, American Association of Variable Star Observers, International Amateur-Professional Photoelectric Photometry (Organization),
1986
10
Eyewitness Companions: Astronomy
LighT curve of cepheid variabLe LighT curve of ecLipsing variabLe. Variable
stars pulsating variables many stars pass through a period of instability at some
point in their lives. T-Tauri stars, which vary in size and brightness as they settle
onto ...
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See the Demon Star Algol 'Wink' in the Night Sky
The so-called "demon star" of Algol is the most prominent eclipsing variable star in the night sky, and if you know when and where to look, you ... «Yahoo News UK, 二月 15»
Challenge Yourself! See an Astronomical Event that Only Happens …
Then you can make refined measurements of eclipsing variable stars. Credit: Brad Timerson/IOTA. But beyond its practical application, we just ... «Universe Today, 一月 15»
Observing Challenge: Catch a Series of Mutual Eclipses by Jupiter's …
What is most apparent during these mutual events is a slow but steady drop in combined magnitude, akin to that of an eclipsing variable star ... «Universe Today, 十一月 14»
This Week's Sky at a Glance, October 10 – 18
High above the Moon and Capella, forming a big triangle with them, is the naked-eye eclipsing variable star Algol. It should be at its minimum ... «Sky & Telescope, 十月 14»
This Week's Sky at a Glance, October 3 – 11
High above the Moon and Capella, forming a big triangle with them, is the naked-eye eclipsing variable star Algol. It should be at its minimum ... «Sky & Telescope, 十月 14»
This Week's Sky at a Glance, September 19–27
The eclipsing variable star Algol (Beta Persei) should be at its minimum light, magnitude 3.4 instead of its usual 2.1, for a couple of hours ... «Sky & Telescope, 九月 14»
This Week's Sky at a Glance, September 12–20
Algol in Perseus, the prototype eclipsing variable star, should be at its minimum light, magnitude 3.4 instead of its usual 2.1, for a couple hours ... «Sky & Telescope, 九月 14»
Mare Nectaris – Credit: Damian Peach
Its formal name is Beta Persei and it is the most famous of all eclipsing variable stars. Tonight, let's identify Algol and learn all about the “Demon ... «Universe Today, 十月 12»
Messier 19 – Credit: Doug Williams, REU Program/NOAO/AURA/NSF
Although this wide pairing is only an optical one, the K-type giant is a double star – an eclipsing variable around 150 times larger than or own ... «Universe Today, 七月 12»
Types of Variable Stars: Cepheid, Pulsating and Cataclysmic
It was an eclipsing variable called Algol, although its variability was not explained until more than a hundred years later by John Goodricke in ... «Space.com, 四月 12»