dwarf spiral galaxy oor Masedonies

dwarf spiral galaxy

Vertalings in die woordeboek Engels - Masedonies

Џуџеста спирална галаксија

en
dwarf version of a spiral galaxy
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It is suggested that dwarf spiral galaxies can transform into dwarf elliptical galaxies, especially in dense cluster environments.
Ова е многу опасен човек, Ваша ВисостWikiMatrix WikiMatrix
Dwarf spiral galaxies, particularly the dwarf counterparts of Sa-Sc type spiral galaxies, are quite rare.
Заборави ги парите!WikiMatrix WikiMatrix
Sm galaxies are typically disrupted and asymmetric. dSm galaxies are dwarf spiral galaxies or dwarf irregular galaxies, depending on categorization scheme.
Звучиш како да си многу, многу зафатенWikiMatrix WikiMatrix
Strong gravitational interactions between galaxies and interactions between galaxies and intracluster gas are expected to destroy the disks of most dwarf spiral galaxies.
Му требаше син, но како замена ме доби менеWikiMatrix WikiMatrix
NGC 5474 NGC 5204 NGC 247 NGC 6503 NGC 3928 NGC 625 NGC 1051 NGC 1311 NGC 2188 IC 4710 Sculptor Dwarf Galaxy Most identified dwarf spiral galaxies are located outside clusters.
Намали Намали за еденWikiMatrix WikiMatrix
Nonetheless, dwarf galaxies with spiral-like structure have been identified within the Virgo Cluster and Coma Cluster.
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The result would be the conversion of (late type) low-luminosity spiral galaxies into dwarf spheroidals and dwarf ellipticals.
Имам фотографија од твоето лицеWikiMatrix WikiMatrix
In contrast, dwarf elliptical galaxies, dwarf irregular galaxies, and the dwarf versions of Magellanic type galaxies (which may be considered transitory between spiral and irregular in terms of morphology) are very common.
Знам, баш и не сака, ама тешко е да и се каже неWikiMatrix WikiMatrix
Dwarf spheroidal galaxies appear to be a distinct class: their properties are more similar to those of irregulars and late spiral-type galaxies.
Проблемите почнаа и пред да стигне овчаротWikiMatrix WikiMatrix
A 2012 paper that suggests a new classification system, first proposed by the Canadian astronomer Sidney van den Bergh, for lenticular and dwarf spheroidal galaxies (S0a-S0b-S0c-dSph) that parallels the Hubble sequence for spirals and irregulars (Sa-Sb-Sc-Im) reinforces this idea showing how the spiral–irregular sequence is very similar to this new one for lenticulars and dwarf ellipticals.
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