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<!DOCTYPE ArticleSet PUBLIC "-//NLM//DTD PubMed 2.7//EN" "https://dtd.nlm.nih.gov/ncbi/pubmed/in/PubMed.dtd">
<ArticleSet>
<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Iranian Journal of Astronomy and Astrophysics</JournalTitle>
				<Issn>2322-4924</Issn>
				<Volume>9</Volume>
				<Issue>2</Issue>
				<PubDate PubStatus="epublish">
					<Year>2022</Year>
					<Month>10</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Instability in the Magnetized Accretion Disks with Outflows in the Presence of Self-Gravity</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>149</FirstPage>
			<LastPage>163</LastPage>
			<ELocationID EIdType="pii">347</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2022.666.1143</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Sekine </FirstName>
					<LastName>Karimzadeh</LastName>
<Affiliation>Department of Physics, Faculty of Sciences, University of Mazandaran, Babolsar, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Alireza </FirstName>
					<LastName>Khesali</LastName>
<Affiliation>Department of Physics, University of Mazandaran Babolsar Iran</Affiliation>

</Author>
<Author>
					<FirstName>Azar </FirstName>
					<LastName>Khosravi</LastName>
<Affiliation>University of Mazandaran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2023</Year>
					<Month>03</Month>
					<Day>14</Day>
				</PubDate>
			</History>
		<Abstract>We study the stability of a model of magnetized accretion disk, in which&lt;br /&gt;outflows play a significant role in driving the inflow, and magnetic field is generated by&lt;br /&gt;a dynamo operating in the disk. We present a local and linear analysis of the stability&lt;br /&gt;in the presence of self-gravity and winds. The numerical results show the model with&lt;br /&gt;self-gravity is unstable in all parts, while in a model without self-gravity, instability&lt;br /&gt;can be observed only in regions near the central body. Eventually, the effect of wind&lt;br /&gt;cooling on the model stability was discussed. According to the results, in systems&lt;br /&gt;without self-gravity, wind cooling can help the system towards stability, but in the&lt;br /&gt;presence of self-gravity, it is shown that our model will remain unstable in all regions.&lt;br /&gt;Comparison of these result with observational evidence shows that this model can be&lt;br /&gt;suitable for the explaining the behavior of the disks surrounding young stellar objects.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">accretion disks</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Outflows</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Instability</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Magnetic fields</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_347_9c9bca287ba1cb00980109e5af54245f.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
