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Towards the Intensity Interferometry Stellar Imaging System
Towards the Intensity Interferometry Stellar Imaging System

... Figure 1: Considering two harmonic emitting points in the source, with slightly different frequencies, telescopes A and B being close together receive beats almost at the same time. This corresponds to a high degree of correlation. Telescopes A and C being further apart do not receive beats in phase ...
Changes in a scientific concept: what is a planet? - Philsci
Changes in a scientific concept: what is a planet? - Philsci

Galileo`s miraculous year: 1609 and the revolutionary telescope
Galileo`s miraculous year: 1609 and the revolutionary telescope

... a brightness of about 9th magnitude compared to the unaided eye’s limit of about 6th magnitude. For comparison, the moons of Jupiter have a brightness between 5th and 6th magnitude. A significant difficulty with the Galilean telescope for astronomy is that the field of view is very narrow. For example ...
CHIRON – A Fiber Fed Spectrometer for Precise Radial Velocities
CHIRON – A Fiber Fed Spectrometer for Precise Radial Velocities

... 5.5◦ in the cross-dispersion direction are the elliptical beam footprint on the camera and the rotation of the slit image by 24◦ . This is compensated by appropriate counter-rotation of the entrance slit, at a cost of cos 24◦ = 0.91 loss in resolution. The light beam emerging from the fiber is tran ...
Alignment Troubleshooting Alignment Procedure
Alignment Troubleshooting Alignment Procedure

... 1. Power on the NexStar by flipping the switch located at the base of the fork are to the on position. 2. Press ENTER to choose Sky Align. Pressing the ALIGN key will bypass the other alignment options and the scrolling text and automatically begins Sky Align. 3. The hand control display will then ...
ancient cultures 114 - Stellenbosch University
ancient cultures 114 - Stellenbosch University

... true astronomical terms, however, a star is a giant ball of gas, constantly undergoing nuclear processes, and as such constantly emitting electromagnetic waves. The light waves produced from these reactions are particularly intense, such that the object can be seen from extremely far away. Our Sun i ...
Stellar Evolution Nucleosynthesis
Stellar Evolution Nucleosynthesis

... • Double-shell burning ends with a pulse that ejects the H and He into space as a planetary nebula. • The PN phase is brief (~104 years) • The core left behind becomes a white dwarf. © 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley ...
The isotopic mixture of barium in the metal-poor
The isotopic mixture of barium in the metal-poor

... the barium resonance line. Our test calculation using the atomic parameters in Kurucz’s library of lines shows that these two features are irrelevant in the case of HD 140283; even if the g f -values are increased by an order of magnitude the pair together cannot contribute more than 0.1 m Å, or ab ...
CHaracterising ExOPlanets Satellite arXiv:1310.7800v1 [astro
CHaracterising ExOPlanets Satellite arXiv:1310.7800v1 [astro

... that can be acquired only by a space-borne observatory and by well understood and mitigated sources of noise. Earth stray light is one of them which becomes the most prominent noise for faint stars. A software suite was developed to evaluate the contamination by the stray light. As the satellite wil ...
Reassessing the formation of the inner Oort cloud
Reassessing the formation of the inner Oort cloud

... either a Hernquist or Plummer potential – and chose other parameters based on the latest observations of embedded clusters from the literature. These other parameters result in the stars being on radial orbits and the cluster collapses. Similar to previous studies, in our simulations the inner Oort ...
Magnificent Cosmos - Academic Program Pages at Evergreen
Magnificent Cosmos - Academic Program Pages at Evergreen

- Spiral - Imperial College London
- Spiral - Imperial College London

... is evidence for both the direct (e.g. Lean et al. 2005; Krivova & Solanki 2008; Krivova et al. 2010; Ball et al. 2011) and inverse (Harder et al. 2009; Preminger et al. 2011) correlations. Lockwood et al. (2007) showed that while the solar 11-year cycle in chromospheric activity is vigorous relative ...
Long-term monitoring of the short period SU UMa
Long-term monitoring of the short period SU UMa

... most cases, are one of the subtypes, characteristic of exhibiting two types of outbursts. One is normal outburst, continuing for a few days. The other is superoutburst, lasting about two weeks, during which modulations called superhumps are shown. The period of the superhumps are a few percent longe ...
The last gasps of VY CMa: Aperture synthesis and adaptive optics
The last gasps of VY CMa: Aperture synthesis and adaptive optics

Silicon isotopic abundance toward evolved stars and its application
Silicon isotopic abundance toward evolved stars and its application

... the local area and raises the pressure, which initiates an expansion and a series of convective and mixing events (Herwig 2005; Iben & Renzini 1983). During the so-called third dredgeup, the products of He burning and the s-process elements are brought to the surface, e.g., 12 C, which can lead to t ...
Emergency Land Navigation
Emergency Land Navigation

... GEM1506K Heavenly Mathematics Advancements in navigational technology have made finding way much easier than before. Nowadays, all kinds of navigational equipment are available, from the basic compass, map, sextant and almanacs to the highly efficient radars and GPS devices. Although technology bri ...
Planet formation
Planet formation

Astronomical Telescope
Astronomical Telescope

... Thus, we now see many commercial telescopes similar to the Maksutov-Cassegrain system illustrated above that packs a long focal length into a physically short tube, while preserving the high-contrast imagery associated with refractors of the same aperture. Catadioptric variations of the Newtonian te ...
Radiative winds, accretion disks and massive stars physics using
Radiative winds, accretion disks and massive stars physics using

Evolution of stars
Evolution of stars

... eclipsed in 2 hours, what is the diameter of the smaller star? a. 175,000 km b. 350,000 km c. 194 km d. 700,000 km e. 4656 km A 2 solar mass star on the main sequence would have a luminosity of approximately __________ solar luminosities. a. 2 b. 4 c. 11 d. 0.5 e. 0.25 Protostars are difficult to ob ...
Lecture ppt - UCO/Lick Observatory
Lecture ppt - UCO/Lick Observatory

... many mirror surfaces. Also throughput to detector goes down. – In astronomy, faint extended objects can actually be harder to see with AO. Limiting factor is sky background, and AO doesn’t improve this for extended objects. Page 30 ...
Multiplicity in Early Stellar Evolution - Astronomy Group
Multiplicity in Early Stellar Evolution - Astronomy Group

... a 100-M⊙ cloud with their AMR MHD code, and found that the magnetic field could reduce the degree of fragmentation, compared to a nonmagnetic cloud collapse, by as much as a factor of 2. Commerçon et al. (2011) extended their previous work on 1-M⊙ clouds to include 100-M⊙ clouds, but again found tha ...
Article PDF - IOPscience
Article PDF - IOPscience

... Using an MSIS model atmosphere,5 we find that this density occurs at a height of 92 km, comparable to the observed height at both AMOR and Arecibo. On the other hand, radar data from Jodrell Bank and from Ottawa show that radar meteoroids detected by those systems also ablate at heights near 95 km ( ...
2 Statistical properties of a sample of periodically variable B-type supergiants
2 Statistical properties of a sample of periodically variable B-type supergiants

3.1 Radio Astronomy Research Results For much of PY 2010, radio
3.1 Radio Astronomy Research Results For much of PY 2010, radio

... around the world have signed on to E@H, of which some fraction is active at any epoch: 1/3 of the active clients receive PALFA data. Data taken with the 100-MHz BW WAPP spectrometers from 2005 to 2009 have been 90% processed with the Cornell code (non-acceleration search), 50% processed with the PRE ...
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