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Photometric properties of type II supernovae

It is shown that late-type spiral galaxies with strong arm populations are by far the main producers of type II supernovae, that no certain type II

Supernovae in dense and dusty environments

Supernova explosions 17 2.1 Iron-core-collapse supernovae Following the the association of CCSNe with the host galaxy spiral arms (e.g

The nuclear bulge of the Galaxy. II. The K band luminosity

represent giants and supergiants which, though they account for only a [1983] for the spiral arm region of the Galactic Disk) may also apply

HI data reduction for the Arecibo Pisces-Perseus Supercluster

the Pisces-Perseus Supercluster to test current supercluster formation models.relates the luminosity to the rotational velocity profile of spiral galaxies

Spiral laser beams in inhomogeneous media

such as oscillating laser beams in a parabolic waveguide and spiral light A similar effect of superfocusing of particle beams in a thin monocrystal

Star formation in N-body simulations. I. The impact of the

for a large sample of spiral galaxies and (we do not yet include supernovae that could which is deter- mined by the Courant-Friedrichs

Curved Cavity Quantum Cascade Laser and Superluminescent

Curved Cavity Quantum Cascade Laser and Superluminescent EmittersTo meet this goal, the first part of this dissertation explores a spiral

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Multifrequency windows on spiral galaxies. 3.Internal

We present aperture photometry data in the H, V, Band U bands of about 100 spiral galaxies belonging to 8 nearby clusters and to the Coma Super

X-ray emission from NGC 4321 (M 100): detection of supernova

In a 42.8 ks ROSAT HRI X-ray observation of the spiral galaxy NGC 4321 (M 100) X-ray emission from the supernova 1979C is discovered, sixteen

Inter-valley spiral order in the Mott insulating state of a

Inter-valley spiral order in the Mott insulating state of a heterostructure graphene-boron nitride Moire super-lattice at half-filling is a Mott

Notes on the Missing Satellites Problem

106L⊙), even when allowing for fairly substantial supernovae feedback. Given that there are only ∼ 10 satellites brighter than this around the Milky

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Heating of Chondritic Materials in Solar Nebula Shocks

Keplerian velocity, so gas orbiting the disk enters the high-density gas of the spiral wave pattern at highly supersonic speeds, which leads to shocks

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The velocity dispersion in giant extragalactic H II regions

Spiral Galaxies, Stellar Mass Ejection, Stellar Winds, B Stars, Galactic Structure, Gas Ionization, Hydrogen Ions, O Stars, Stellar Evolution, Supersonic

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Coronal Mass Ejection Shock and Sheath Structures Relevant to

which expands outward at supersonic speeds, forming the solar wind (Parkerspiral, causing the field to grow ever more perpendicular to the shock

Radioactive 26Al from massive stars in the Galaxy

Supplementary Discussion: Star Formation Rate (SFR) and Supernova Rate (SNR(Elect…); these encode the spiral structure of the Galaxy; different

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falcónbarroso jesús - Secular Evolution of Galaxies

supernova explosions; since the supernova rate is directly related to the the UV light in the inter-arm regions of spiral galaxies displays a

Three-dimensional spiral antenna and applications thereof

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Matter in a One Parameter Extension of the Minimal Super

spiral galaxies [22], and whose density profile reads ρB (r) = (1 +Within the minimal supergravity model (mSUGRA) framework, the expectation for

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Adaptation to spiral motion: global but not local motion

When superimposed, all contours of the spiral stimulus and its mirror image are 90 degrees apart. Presenting the same spiral during the test period shows