variable star oor Bengaals

variable star

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(astronomy) Any star whose brightness varies.

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বিষমতারা

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star whose brightness as seen from Earth fluctuates
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The Sun is not considered a variable star, but it does undergo periodic changes in activity known as the sunspot cycle.
যে কনসোল-এর ট্যাব-বার-এ " নতুন " বাটনটি ব্যবহার করে আপনি নতুন সেশন শুরু করতে পারেন?WikiMatrix WikiMatrix
The records of the American Association of Variable Star Observers (AAVSO) show a maximum brightness of 0.2 in 1933 and 1942, and a minimum of 1.2, observed in 1927 and 1941.
গ্রিড/ছক প্রদর্শন বা আড়াল করো ।WikiMatrix WikiMatrix
Loading Variable Stars
এই বিন্দু দিয়ে একটি অর্ধ-রেখা আঁকোSamanantar Samanantar
variable star
& অডিও ডিভাইস বেছে নিনSamanantar Samanantar
Most of the contributions of Radhagovinda were related to variable stars.
এখানে & কপি করোSamanantar Samanantar
Light Curve produced by the American Amateur Variable Star Observers
যতিচিহ্ন, উদ্ধৃতি সমাপ্তিSamanantar Samanantar
A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.
উইণ্ডোটি সরাওSamanantar Samanantar
"It is from the title of this book that the modern word ""nova"" for cataclysmic variable stars is derived."
ফাইল অন্তর্ভুক্ত করোSamanantar Samanantar
"It is from the title of this book that the modern word ""nova"" for cataclysmic variable stars is derived."
আমার স্বামী জোয়ি আধ্যাত্মিক সাহায্য জুগিয়ে আমাকে সামলেছিলেন।Samanantar Samanantar
It may be mentioned that Radhagovinda observed 37215 Variable stars from 1919 to 1954 and dispatched data on those to .
ডিস্কের কোটা পেরিয়ে গেছেSamanantar Samanantar
"""The Sun is not considered a variable star, but it does undergo periodic changes in activity known as the sunspot cycle"""
তিনি এই বিয়ে খেতে এসেছেন ।Samanantar Samanantar
Five known variable stars lie within the broadest radius, the tidal radius, of it, all of which are RR Lyrae variables.
ঝড়ের সাথে ব্যাপক বৃষ্টিপাত এই দেশে স্মরণকালের সবচেয়ে ভয়াবহ বন্যার সৃষ্টি করেছে।Samanantar Samanantar
Although the categorisation of variable star types is increasingly done from their spectral properties, the amplitudes, periods, and regularity of their brightness changes are still important factors.
অ্যাকাউন্ট তৈরি করতে অক্ষমSamanantar Samanantar
published a role of honour in June 1946. It included names of Leading 25 astronomers of the world including Radhagovinda Chandra, who observed over ten thousand variable star, comets etc.
ডিফল্ট স্কোর জন্য অগ্রাহ্য করাSamanantar Samanantar
An accurate determination of the distance to the Galactic Center as established from variable stars (e.g. RR Lyrae variables) or standard candles (e.g. red-clump stars) is hindered by countless effects, which include: an ambiguous reddening law. a bias for smaller values of the distance to the Galactic Center because of a preferential sampling of stars toward the near side of the Galactic bulge owing to interstellar extinction. and an uncertainty in characterizing how a mean distance to a group of variable stars found in the direction of the Galactic bulge relates to the distance to the Galactic Center.
স্ক্যান ফোল্ডারSamanantar Samanantar
The concept of momentum plays a fundamental role in explaining the behavior of variable-mass objects such as a rocket ejecting fuel or a star accreting gas.
থাইল্যান্ডের প্রধানমন্ত্রী অভিশিত ভিজ্জাজেভা ঘোষণা দেন যে এই ওয়েব সাইটের উদ্দেশ্য দেশটির ইমেজ বা চেহারা আবার ঠিক করা এবং সম্প্রতি কালে যে অস্থিরতা চলছে তার প্রেক্ষাপটে জাতিকে এক করা।Samanantar Samanantar
"The nature of the Milky Way's bar, which extends across the Galactic Center, is also actively debated, with estimates for its half-length and orientation spanning between 1-5 kpc (short or a long bar) and 10-50. Certain authors advocate that the Milky Way features two distinct bars, one nestled within the other. The bar is delineated by red-clump stars (see also red giant). however, RR Lyr variables do not trace a prominent Galactic bar. The bar may be surrounded by a ring called the ""5-kpc ring"" that contains a large fraction of the molecular hydrogen present in the Milky Way, as well as most of the Milky Way's star formation activity. Viewed from the Andromeda Galaxy, it would be the brightest feature of the Milky Way."
অপর বিন্দু দুটির অন্যটি বেছে নিনSamanantar Samanantar
Microquasars are named after quasars, as they have some common characteristics: strong and variable radio emission, often resolvable as a pair of radio jets, and an accretion disk surrounding a compact object which is either a black hole or a neutron star.
শিশুর সময়-সংরক্ষকSamanantar Samanantar
The variability of HMXBs are observed in the form of X-ray pulsars and not X-ray bursters. These X-ray pulsars are due to the accretion of matter magnetically funneled into the poles of the compact companion. The stellar wind and Roche lobe overflow of the massive normal star accretes in such large quantities, the transfer is very unstable and creates a short lived mass transfer.
স্তর সংক্রান্ত পরিসংখ্যানSamanantar Samanantar
A microquasar (or radio emitting X-ray binary) is the smaller cousin of a quasar. Microquasars are named after quasars, as they have some common characteristics: strong and variable radio emission, often resolvable as a pair of radio jets, and an accretion disk surrounding a compact object which is either a black hole or a neutron star. In quasars, the black hole is supermassive (millions of solar masses). in microquasars, the mass of the compact object is only a few solar masses. In microquasars, the accreted mass comes from a normal star, and the accretion disk is very luminous in the optical and X-ray regions. Microquasars are sometimes called radio-jet X-ray binaries to distinguish them from other X-ray binaries. A part of the radio emission comes from relativistic jets, often showing apparent superluminal motion.[citation needed]
সকল নির্বাচন বাতিল করSamanantar Samanantar
20 sinne gevind in 11 ms. Hulle kom uit baie bronne en word nie nagegaan nie.