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1 Markets I: The Ecosystem and Exchange-Traded Marketsবাজার অনলাইন 2 Markets II: Rates, FX and Creditবাজার অনলাইন 3 Markets III: Commodities, Energy and Cryptoবাজার অনলাইন 4 Quantitative Methodsপদ্ধতি অনলাইন 5 Derivatives and Volatilityডেরিভেটিভস অনলাইন 6 Rates, Credit, XVA and Riskসুদহার, ঋণ ও ঝুঁকি অনলাইন 7 Research Craft: Predictors, Backtests, Measurement, Portfoliosগবেষণা অনলাইন 8 Strategies I: Equities and Futuresকৌশল অনলাইন 9 Strategies II: Volatility, Relative Value, Macro and the Bank Desksকৌশল অনলাইন 10 Microstructure and Executionএক্সিকিউশন অনলাইন 11 Market Making and High-Frequency Tradingমার্কেট মেকিং অনলাইন 12 Machine Learning for Marketsমেশিন লার্নিং অনলাইন 13 Low-Latency Softwareপ্রযুক্তি অনলাইন 14 Networks, Hardware and Trading Infrastructureপ্রযুক্তি অনলাইন 15 Research, Data and Risk Platformsপ্রযুক্তি অনলাইন 16 The Desk and the Firmপ্রতিষ্ঠান অনলাইন 17 The Industry: Firms, Roles and Careersক্যারিয়ার অনলাইন 18 Interviews I: Maths, Probability and Speedক্যারিয়ার অনলাইন 19 Interviews II: Markets, Trading Games and the Final Roundক্যারিয়ার অনলাইন 20 Interviews III: Codeক্যারিয়ার অনলাইন
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Earth and Space Sciences · পরিভাষা

Galactic disc, thick disc, bulge and stellar halo কী?

অন্য নাম: Galactic disc · thick disc · Galactic bulge · stellar halo

Definition 29.1 University Earth and Space Sciences — Year 3 · অধ্যায় 29 — The Milky Way and Galaxies

The Galactic disc is the flattened component of the Galaxy, made of stars, gas and dust in nearly circular orbits about its centre; its density falls off roughly exponentially with height above its mid-plane and with distance from its centre, over a scale height and a scale length. The thick disc is a second, older disc component of larger scale height and smaller mass. The Galactic bulge is the central concentration of stars that swells out of the disc. The stellar halo is the sparse, roughly spheroidal component of old stars and globular clusters that surrounds the disc and the bulge.

A sketch of the Galaxy, to scale for its main dimensions. (a) Edge-on: the thin disc (dark band), the thick disc (light band), the box-shaped bulge, and the stellar halo with its globular clusters (orange dots); the Sun lies in the disc, about 8.2\, kpc from the centre and about 25\, pc above the mid-plane (too small to show). (b) Seen from the north Galactic pole: the bar, about 5\, kpc in half-length, tilted by 27 to the line from the Sun to the centre (dotted); the solar circle (dashed); spiral arms drawn schematically; the Galaxy turns clockwise in this view.
A sketch of the Galaxy, to scale for its main dimensions. (a) Edge-on: the thin disc (dark band), the thick disc (light band), the box-shaped bulge, and the stellar halo with its globular clusters (orange dots); the Sun lies in the disc, about 8.2 kpc8.2\,\mathrm{kpc} from the centre and about 25 pc25\,\mathrm{pc} above the mid-plane (too small to show). (b) Seen from the north Galactic pole: the bar, about 5 kpc5\,\mathrm{kpc} in half-length, tilted by 27∘27{}^{\circ} to the line from the Sun to the centre (dotted); the solar circle (dashed); spiral arms drawn schematically; the Galaxy turns clockwise in this view.
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