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3D Simulations of Low-Mass Proto-Stellar Disks With Certain Initial Conditions Using Smoothed Particle Hydro Dynamics

Thesis Info

Access Option

External Link

Author

Riaz, Rafeel

Program

PhD

Institute

University of Karachi

City

Karachi

Province

Sindh

Country

Pakistan

Thesis Completing Year

2016

Thesis Completion Status

Completed

Subject

Physics

Language

English

Link

http://prr.hec.gov.pk/jspui/bitstream/123456789/13286/1/Rafeel_Riaz_Astrophysics_2016_HSR_univ_of_Karachi_25.08.2016.pdf

Added

2021-02-17 19:49:13

Modified

2024-03-24 20:25:49

ARI ID

1676725390195

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Results of the numerical study on the initial formation stages of low-mass protostellar systems leading to single, binary, triplet, and quadruple protostar systems formation are reported here. In addition to these various types of protostellar objects we also investigate the overall structure formation that takes place within collapsing molecular cores that yield during the course of evolution the spiral structure formation, ring formation, and bar formation under various initial conditions chosen for a rotating solar mass cloud of molecular hydrogen to mimic the states prevailing in star formation regions in our Milky Way galaxy. There have been three key parameters belonging to the initial star forming conditions whose effects on the overall outcome of protostallar systems have been examined. These parameters are the initial thermal state of the prestellar core, the amplitude of azimuthal density perturbation introduced in initially uniform density state of the core, and the impact of the critical density which governs the transition from isothermal to adiabatic thermodynamic behavior of the collapsing core. For protostellar binaries, the separation is determined as a function of the initial thermal state of the core by varying its initial temperature. For this purpose a slightly modified version of the Burkert and Bodenheimer collapse test is taken into consideration. We find that the result is fairly sensitive to both the initial thermal state of the cloud and the initial azimuthal density perturbation’s amplitude A. For A=10 %, variations of only 1 unit Kelvin below 10 K causes a change of up to 100 AU in protobinary separation, while for this small amplitude of perturbation the initial temperatures above 10 K result a single low-mass fragment, instead of a binary, that does not reach even near to the protostellar densities. However, protostellar binaries, do appear if the amplitude of perturbation is enhanced from 10 % to 25 %. A star forming hydrogen gas is normally considered to be initially at 10 K. For structural formation study, we have explored that an oscillation around this normally considered value can be influential in determining the fate of a collapsing gas as it evolves in its structural properties that may lead to formation of proto-stars. We examined the initial range of temperature of star forming gas between 8 K to 12 K and tried to compare the emerging physical properties within the early phase of formation of protostellar system. According to our findings the spiral structures are likely to appear in a strongly perturbed molecular cores that commence their phase of collapse from temperatures lesser than 10 K. However, cores with initial temperatures more than 10 K potentially develop, instead of spiral, a ring structure which afterwards experiences the clumps formation. It is possible to observe a transition from spiral to ring instability at a typical initial core temperature of 10 K. Similarly, while investigating the effects of critical density variations on the evolution of protostellar systems, we find that the critical density affects the structural evolution of the envelope of gas, also the dimension of emerging rotating disk structures during collapse too get affected as well as the number of fragments appearing from the concluding fragmentation of the disks. It is suggested that this mechanism has the potential to give birth to young protostellar objects that may eventually constitute systems of bound multiple protostars. The entire numerical experiment is conducted by using 250025 SPH particles to construct virtually the geometry of each molecular core investigated here.
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ماں دی ممتا

ماں دی ممتا

پرانے زمانے دی گل اے کہ اک پنڈ دے لوک بہت ای ظالم سن۔ خاص طور تے اوہ پرندیاں دا شکار کردے۔ درختاں اتے چڑھ کے اوہناں دے آہلنیاںوچوں انڈے یاں بچے کڈھ لیندے سن۔ ایس پنڈ دے باہر اک بہت وڈا بوڑھ دا درخت سی۔ اوتھے اک طوطے نے آہلنا پایا۔ اک طوطا تے طوطی گلاں کردے نیں طوطا طوطی نوں آکھدا اے:

طوطیے من موتیے ایس نگری نہ جا

ایس نگری دے جٹ برے نیں پھائیاں لیندے پاء

اگوں طوطی جواب دیندی اے:

طوطیا من موتیا ٹاہلی میرے بچڑے لک ٹنوں ٹنوں

اوہناں دے دو چھوٹے بچے وی ہوندے نیں۔ طوطا آکھدا اے کہ میں پنڈ جاندا ہاں تاں جے بچیاں لئی کجھ کھاون لئی لے آواں۔ طوطی آکھدی اے۔

طوطیا من موتیا ٹاہلی میرے بچڑے لک ٹنوں ٹنوں

میں اپنے بچیاں نوں چھڈ کے نئیں جا سکدی جے میرے بچیاں نوں کجھ ہو گیا تاں میرا لک ٹٹ جاوے گا۔ میں مر جاواں گی۔ طوطا جان لگدا اے تے طوطی آکھدی اے۔ کہ توں ایس نگری نہ جا۔ ایس نگری دے لوک بہت برے نیں۔ اوہ تینوں قید کر لین گے تے جے تینوں کجھ ہو گیا تاں ساڈا کیہ بنے گا۔ طوطا ایہہ گل سن کے چپ کر کے بہہ جاندا اے۔ اوہ ٹاہلی تے بیٹھے ہوندے نیں تے جیہڑا وی مسافر ٹاہلی دے کولوں لنگھ دا اے۔ اوہ ایہو آکھدی اے۔

ٹاہلی میرے بچڑے لک ٹنوں ٹنوں

اک دن اک راہ گیر دھپ توں بچن لئی ٹاہلی تھلے بہہ جاندا اے۔ اوہدے کول روں ہوندا اے۔ طوطی روں ویکھ کے اوس نوں آکھدی اے۔

الشيخ علي الطنطاوي وخدماته العلمية والأدبية

There is no doubt that Sheikh Ali-al Tantāwi is one of the most prominent ،famous and best writers and preachers of Islam in the modern era. He is one of the pioneers of Islamic literature, he is also a talented writer and a good social reformer. He has left great heritage of Islamic sciences and literature for us. In this article we have tried to emerge the different aspects of his life and services in the field of society reforms، literature، preaching and journalism.

Palynological Investigation of Allergenic and Melliferous Flora of Pakistan

The microscopic analysis of pollen is the standard method and an effective tool to understand the allergenic (Pollen allergy) and melliferous plants (mellisopalynology) of any specific region. This is the first report study from Pakistan regarding pollen investigation of allergenic and melliferous flora using various techniques including pollen extraction, identification, systematics, field emission scaning electron microscopy, upright florescence microscopy and light microscopy. The study confind palynological analysis of melliferous plants and allergenic plants, pollen sculpturing using scaning electron micrscopy and to development of floral calendar of the region. First part deals with pollen analysis of 64 honey samples collected from 37 different localities of Pakistan using Light microscopy (LM) and Field Emission Scanning Electron Microscope (FESEM). In this study wide variety of plants foraged by honey bees Apis mellifera, A. cerana, A. dorsata were identified representing the potential for bee keeping of region. In total of 60 different pollen types belonging to 35 families were identified up to species, genetic and family level. It is reported that the most of the plants belong to angiosperm families whereas only one species belong to gymnosperm group.The dominant families belonging to angiosprm includes Brassicaceae, Rosaceae, Rutaceae, Apiaceae, Lamiaceae, Boraginaceae, Mimosaceae whereas the pinaceae is the only one gymnospermic family. In second part, Upright fluorescence microscopy was carried out to identify 12 samples of allergenic pollen from Pakistan. Pollen focal series has been capture at different dimensions expressing the diverse features of pollen, significant for aerobiological sampling identification. Pollen features studied includes pollen morphology, size, shape, exine structure, exine thickness etc. Diverse pollen morphology observed during study may appear confusing when working on airborne pollen as many pollen show similarity in shape. Third part deals with Field emission scanning electron microscopy (FESEM) of pollen grain. Finding of this analyses shows that the external morphological features of pollen (sculpturing) were useful for identification of different taxa. Honey pollen were identified using morphological features, number and arrangement of pore and colpi, size and shape. In this study 49 pollen grains types belonging to 25 families were reported. It is noted that the shape and sculpturing of pollen ranging from psilate, scabrate to reticulate, bireticulate and echinolophate. Survey of allergenic and melliferous flora was carried out side by side to keep the record about allergenic and bee floral preference of specific sites through surveys and interviews and recording their flowering time and distribution. In total of 205 plant species were identified belonging to sixty seven families. The wild plant species like Justicia adhatoda Linn., Acacia nilotica (L.) Delile, Ziziphus jujuba Mill etc. may serve in apiculture industries at large scale while the species like Taraxicum officinalis L., Artemisia dubia Wall., Casuarina equisetifolia L., Broussonetia papyrifera (L.) L’Herit., Cupressus sempervirens L., or Pinus roxburghii Sargent, playing role in triggering pollen allergy symptoms. Cultivated crops like Pennisetum, Nigella sativa, Triticum sativum along with fruit gardens of Pyrus spp., Prunus spp., Eryobotria japonica, Citrus spp. etc. are popular melliferous flora of studied sites. Exotic/ introduced species like Eucalyptus globulus or Parthenium hysterophorus, are also frequently visited by bees indicating the significance of those plants in bee industry and at the same time triggering the allergies by the windborne pollen. Overall results are based on pollen features like morphology and sculpturing. It is concluded that different microscopic analysis techniques gives more clear and authentic picture of allergenic and melliferous pollen identification which is well supported by floral calendar. Diversity of pollen are observed in case of melliferous pollen and most of the allergenic pollen were found less sculptured or psilate expressing the adaptation to the specific mode of pollination. The study recommends to compile the pollen book on pollen spectra of Pakistan that could serve as a reference for future studies particularly and at global perspectives generally.