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Dark Matter: A Brief Review
Dark Matter: A Brief Review

Globular and Open Clusters in our Galaxy
Globular and Open Clusters in our Galaxy

double slit interference
double slit interference

... (2) Division of Amplitude: In this method, the amplitude of the incoming beam is divided into two or more parts by partial reflection with the help of mirrors, lenses and prisms. These divided parts travel different paths and finally brought together to produce interference. The common methods are a ...
THE GREAT AGN DEBATE `AGN VS STARBURST
THE GREAT AGN DEBATE `AGN VS STARBURST

TDE in the XMM-Newton slew survey
TDE in the XMM-Newton slew survey

The Historical X-ray Transient KY TrA in quiescence
The Historical X-ray Transient KY TrA in quiescence

Architectural Caustics — Controlling Light with Geometry
Architectural Caustics — Controlling Light with Geometry

Galaxy Pairs in the Sloan Digital Sky Survey
Galaxy Pairs in the Sloan Digital Sky Survey

The stellar populations in the low-luminosity, early
The stellar populations in the low-luminosity, early

Post-starburst galaxies: more than just an interesting curiosity
Post-starburst galaxies: more than just an interesting curiosity

variable star type designations in vsx
variable star type designations in vsx

... minima may be absent. An extremely wide range of periods is observed, from 0.2 to ≥10000 days. Light amplitudes are also quite different and may reach several magnitudes. EB β Lyrae-type eclipsing systems. These are eclipsing systems having ellipsoidal components and light curves for which it is imp ...
Substellar Objects in Nearby Young Clusters (SONYC) VI: The
Substellar Objects in Nearby Young Clusters (SONYC) VI: The

Eclipse Box Activity Guide - Girl Scouts of Northern California
Eclipse Box Activity Guide - Girl Scouts of Northern California

Cosmological  Constraints from  the  Virial  Mass
Cosmological Constraints from the Virial Mass

... ster.), which is necessary given the low redshift limit of the survey. I acquire optical redshifts for the target galaxies in R2FGS from the literature and from new data collected with the FAST spectrograph on Mt. Hopkins. After removing foreground and background galaxies (interlopers) using a dynam ...
Effects of Light Intensity, Illumination Cycles on Microalgae
Effects of Light Intensity, Illumination Cycles on Microalgae

Dark matter scaling relations and the assembly epoch of Coma early
Dark matter scaling relations and the assembly epoch of Coma early

pitfall prevention
pitfall prevention

... The field of geometric optics involves the study of the propagation of light, with the assumption that light travels in a fixed direction in a straight line as it passes through a uniform medium and changes its direction when it meets the surface of a different medium or if the optical properties of ...
Light and Color - IA
Light and Color - IA

The low dark matter content of the lenticular galaxy NGC 3998
The low dark matter content of the lenticular galaxy NGC 3998

Evidence for strong evolution in galaxy environmental quenching
Evidence for strong evolution in galaxy environmental quenching

The European Large Area ISO Survey – IV. The preliminary 90
The European Large Area ISO Survey – IV. The preliminary 90

KIC 8462852 Faded Throughout the Kepler Mission
KIC 8462852 Faded Throughout the Kepler Mission

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THE EVOLUTION OF GALAXY NUMBER DENSITY AT Z < 8 AND
THE EVOLUTION OF GALAXY NUMBER DENSITY AT Z < 8 AND

MUFASA: The assembly of the red sequence
MUFASA: The assembly of the red sequence

... Mufasa is heuristic and requires free parameters. In our case the key free parameter is the quenching halo mass scale, i.e. the halo mass above which we keep halo gas hot. To choose this, we appeal to constraints derived from the analytic equilibrium model for galaxy evolution (Mitra, Davé, & Finla ...
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Gravitational lens

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