HABITAT.pptx
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The document discusses different types of habitats including aquatic, terrestrial, and arboreal habitats. It provides examples of organisms found in each habitat and describes their adaptations. Aquatic habitats include freshwater, marine, and estuarine environments inhabited by organisms like whales, turtles, and water plants. Terrestrial habitats refer to land environments where organisms such as humans, domestic animals, and wild animals live. Arboreal habitats refer to life in or on trees and are home to animals like parrots and monkeys. The document then discusses examples of adaptations that allow organisms to survive in their habitats, such as gills and fins in aquatic organisms, extensive root systems in terrestrial plants, and wings in arboreal birds and bats.
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Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
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a compound pendulum is a physical system with a more complex structure than a simple pendulum, incorporating its mass distribution and dimensions into its oscillatory motion around a fixed axis. Understanding its dynamics involves principles of rotational mechanics and the interplay between gravitational potential energy and kinetic energy. Compound pendulums are used in various scientific and engineering applications, such as seismology for measuring earthquakes, in clocks to maintain accurate timekeeping, and in mechanical systems to study oscillatory motion dynamics.
Embracing Deep Variability For Reproducibility and Replicability
Embracing Deep Variability For Reproducibility and ReplicabilityUniversity of Rennes, INSA Rennes, Inria/IRISA, CNRS
Embracing Deep Variability For Reproducibility and Replicability
Abstract: Reproducibility (aka determinism in some cases) constitutes a fundamental aspect in various fields of computer science, such as floating-point computations in numerical analysis and simulation, concurrency models in parallelism, reproducible builds for third parties integration and packaging, and containerization for execution environments. These concepts, while pervasive across diverse concerns, often exhibit intricate inter-dependencies, making it challenging to achieve a comprehensive understanding. In this short and vision paper we delve into the application of software engineering techniques, specifically variability management, to systematically identify and explicit points of variability that may give rise to reproducibility issues (eg language, libraries, compiler, virtual machine, OS, environment variables, etc). The primary objectives are: i) gaining insights into the variability layers and their possible interactions, ii) capturing and documenting configurations for the sake of reproducibility, and iii) exploring diverse configurations to replicate, and hence validate and ensure the robustness of results. By adopting these methodologies, we aim to address the complexities associated with reproducibility and replicability in modern software systems and environments, facilitating a more comprehensive and nuanced perspective on these critical aspects.
https://hal.science/hal-04582287
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Methods of grain storage Structures in India.pdf
•Post-harvestlossesaccountforabout10%oftotalfoodgrainsduetounscientificstorage,insects,rodents,micro-organismsetc.,
•Totalfoodgrainproductioninindiais311milliontonnesandstorageis145mt.InIndia,annualstoragelosseshavebeenestimated14mtworthofRs.7,000croreinwhichinsectsaloneaccountfornearlyRs.1,300crores.
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Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
Synopsis presentation VDR gene polymorphism and anemia (2).pptx
I am the PhD scholar of FND department, Assam down town University
Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS
+
53.13485
−
27.82088
with a host spectroscopic redshift of
2.903
±
0.007
. The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red (
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∼
0.9
) despite a host galaxy with low-extinction and has a high Ca II velocity (
19
,
000
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2
,
000
km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low-
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Ca-rich population. Although such an object is too red for any low-
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cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement (
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1
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) with
Λ
CDM. Therefore unlike low-
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Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high-
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truly diverge from their low-
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counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.
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22PH503 - Astronomy and Astrophysics - Unit 2 - Spectral Classification of Stars
Undergrad Physics - BSc Physics
Post translation modification by Suyash Garg
overview of PTM helps to the students who wants to clear their basics about it.
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Quality assurance B.pharm 6th semester BP606T UNIT 5
Quality assurance B.pharm 6th semester BP606T UNIT 5
22PH503 - Astronomy and Astrophysics - Unit 2 - Spectral Classification of Stars
22PH503 - Astronomy and Astrophysics - Unit 2 - Spectral Classification of Stars
HABITAT.pptx
- 1. HABITAT
- 2. Habitat is a place or environment where organisms normally live. There are three major types of habitat. These are : Aquatic terrestrial arboreal habitats.
- 3. Aquatic Habitat: (i) Freshwater (ii) Marine (iii) Estuarine Living organisms found living in aquatic habitat include whale, turtles, water lettuce, water lilies etc. Aquatic habitats are classified according to their salinity (salt content).
- 4. Terrestrial Habitat: • Then terrestrial habitat refers to land environment. Living organisms found living in terrestrial habitat include man, domestic animals e.g. dog, cat, goat, wild animals such as lion, tiger etc. Terrestrial habitats can be; • (i) Tropical rainforest • (ii) Savannah (grassland) • (iii)Desert
- 5. Arboreal Habitat: Arboreal habitat means air environment. It can also be referred to as life in or on trees habitat. Animals like parrots, weaver birds, monkeys and orangutans are good examples of animals found in arboreal habitats.
- 6. ADAPTATION OF ORGANISMS TO THEIR HABITATS Plants and animals are found in a particular area (habitat) because they have special features which help them to survive in that habitat. Adaptation is any feature of an organism in structure or activity that makes the organism to survive in its environment. Such features are called adaptive features. For instance, fishes have gills, fins and tails (adaptive features) water bodies.
- 7. ADAPTATION OF PLANTS TO AQUATIC HABITAT; (i) They have poorly developed root system. (ii) Generally, leaves of aquatic plants have large air spaces that keep them buoyant and let them absorb oxygen. (iii) Some possess breathing roots for gaseous exchange. (iv) Some possess waxy cuticles on their leaves to prevent wetting so that gaseous exchange can easily take place. Plants which grow only in or on water are known as hydrophytes e.g. Water lettuce, Water Lily.
- 8. ADAPTATION OF PLANTS TO TERRESTRIAL HABITAT; (i) They possess extensive root system for anchorage and water absorption e.g. Mahogany. (ii) Desert plants possess tiny and scanty leaves to reduce water loss through transpiration. (iii) Some have leaves reduced to spines e.g. Cactus, to reduce the rate of transpiration. (iv) They possess thick bark on their stems to protect internal tissues. (v) Some have special storage tissues that enable them to withstand conditions of external drought by using their water storage. E.g. Cactus.
- 9. ADAPTATION OF ANIMALS TO THEIR HABITATS Habitats Adaptation Living Organisms Aquatic Fins and tails for swimming, streamlined body for swimming. Fish, Toad, Tadpoles Webbed feet for swimming. Duck, Toads, Crocodile, Frog etc. Gills for breathing. Fish, Tadpoles Terrestrial Limbs, legs, arms, feet for walking, running and jumping, lung for breathing Man, Dog, Cow, Rat, lion etc Scaly skin to reduce water loss. Lizard Arboreal Wings for flight. Birds, Bat, Insects etc.
- 10. Slide Title Product A • Feature 1 • Feature 2 • Feature 3 Product B • Feature 1 • Feature 2 • Feature 3
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