Loading…
UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring
Results of a long-term (17 years) photometric monitoring of five T Tau stars in the VRI bands are presented. All the studied objects are members of the young cluster IC 348 and show the UX Ori type variability caused by changes in the circumstellar extinction. Three of them (V712 Per, V716 Per, and...
Saved in:
Published in: | Astrophysics 2022-09, Vol.65 (3), p.368-383 |
---|---|
Main Authors: | , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | cdi_FETCH-LOGICAL-c301t-a5b817cdb7278282833941738bffecab68d62f1e6dbf698e266d07c55e7108b13 |
container_end_page | 383 |
container_issue | 3 |
container_start_page | 368 |
container_title | Astrophysics |
container_volume | 65 |
creator | Barsunova, O. Yu Grinin, V. P. Sergeev, S. G. Shugarov, S. Yu Efimova, N. V. Nazarov, S. V. |
description | Results of a long-term (17 years) photometric monitoring of five T Tau stars in the VRI bands are presented. All the studied objects are members of the young cluster IC 348 and show the UX Ori type variability caused by changes in the circumstellar extinction. Three of them (V712 Per, V716 Per, and V909 Per) are classical T Tau type stars (CTTS) and the other two (V695 Per, V715 Per) are weak-line T Tauri stars (WTTS). Their light curves demonstrate the large diversity. Three of the objects have a combination of two different types of activity: stochastic UX Ori type variability and periodic brightness variations similar to those observed in AA Tau stars. Two of the stars demonstrate only the stochastic brightness variations owing to fluctuations in circumstellar extinction at different characteristic times. The features of the photometric activity of the stars investigated are discussed in detail in this article. |
doi_str_mv | 10.1007/s10511-022-09747-x |
format | article |
fullrecord | <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_journals_2733387336</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A728631738</galeid><sourcerecordid>A728631738</sourcerecordid><originalsourceid>FETCH-LOGICAL-c301t-a5b817cdb7278282833941738bffecab68d62f1e6dbf698e266d07c55e7108b13</originalsourceid><addsrcrecordid>eNp9kV1LIzEUhoOsYFf9A14F9mov4uajk2T2TsqqhS6KVvAuzGROaqQz6SYZqP_e1C5IYVkOnEB4nhxyXoQuGL1klKofidGKMUI5J7RWU0W2R2jCKiWIZjX7gia0UowoXskT9DWlV0ppLWs5QcunZ3wX53j5tgH8mJuYsB9wfgE8W48pQ8TzGRZT_RM_QBrXOeHg8CIMK7KE2OP7l5BDDzl6i3-HwecQ_bA6Q8euWSc4_3ueoqfrX8vZLVnc3cxnVwtiBWWZNFWrmbJdq7jSvJQQ9ZQpoVvnwDat1J3kjoHsWidrDVzKjipbVaAY1S0Tp-jb_t1NDH9GSNm8hjEOZaThSgihS5Of1KpZg_GDCzk2tvfJmivFtRS7kYW6_AdVqoPe2zCA8-X-QPh-IBQmwzavmjElM398OGT5nrUxpBTBmU30fRPfDKNmF6DZB2hKgOYjQLMtkthLabNbKsTP3_3HegcA5Znm</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2733387336</pqid></control><display><type>article</type><title>UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring</title><source>Springer Nature</source><creator>Barsunova, O. Yu ; Grinin, V. P. ; Sergeev, S. G. ; Shugarov, S. Yu ; Efimova, N. V. ; Nazarov, S. V.</creator><creatorcontrib>Barsunova, O. Yu ; Grinin, V. P. ; Sergeev, S. G. ; Shugarov, S. Yu ; Efimova, N. V. ; Nazarov, S. V.</creatorcontrib><description>Results of a long-term (17 years) photometric monitoring of five T Tau stars in the VRI bands are presented. All the studied objects are members of the young cluster IC 348 and show the UX Ori type variability caused by changes in the circumstellar extinction. Three of them (V712 Per, V716 Per, and V909 Per) are classical T Tau type stars (CTTS) and the other two (V695 Per, V715 Per) are weak-line T Tauri stars (WTTS). Their light curves demonstrate the large diversity. Three of the objects have a combination of two different types of activity: stochastic UX Ori type variability and periodic brightness variations similar to those observed in AA Tau stars. Two of the stars demonstrate only the stochastic brightness variations owing to fluctuations in circumstellar extinction at different characteristic times. The features of the photometric activity of the stars investigated are discussed in detail in this article.</description><identifier>ISSN: 0571-7256</identifier><identifier>EISSN: 1573-8191</identifier><identifier>DOI: 10.1007/s10511-022-09747-x</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Astronomy ; Astrophysics ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Brightness ; Clusters ; Extinction ; Light curve ; Monitoring ; Observations and Techniques ; Photometry ; Physics ; Physics and Astronomy ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Star brightness ; Stars ; T Tauri stars ; Variability</subject><ispartof>Astrophysics, 2022-09, Vol.65 (3), p.368-383</ispartof><rights>Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><rights>COPYRIGHT 2022 Springer</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c301t-a5b817cdb7278282833941738bffecab68d62f1e6dbf698e266d07c55e7108b13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Barsunova, O. Yu</creatorcontrib><creatorcontrib>Grinin, V. P.</creatorcontrib><creatorcontrib>Sergeev, S. G.</creatorcontrib><creatorcontrib>Shugarov, S. Yu</creatorcontrib><creatorcontrib>Efimova, N. V.</creatorcontrib><creatorcontrib>Nazarov, S. V.</creatorcontrib><title>UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring</title><title>Astrophysics</title><addtitle>Astrophysics</addtitle><description>Results of a long-term (17 years) photometric monitoring of five T Tau stars in the VRI bands are presented. All the studied objects are members of the young cluster IC 348 and show the UX Ori type variability caused by changes in the circumstellar extinction. Three of them (V712 Per, V716 Per, and V909 Per) are classical T Tau type stars (CTTS) and the other two (V695 Per, V715 Per) are weak-line T Tauri stars (WTTS). Their light curves demonstrate the large diversity. Three of the objects have a combination of two different types of activity: stochastic UX Ori type variability and periodic brightness variations similar to those observed in AA Tau stars. Two of the stars demonstrate only the stochastic brightness variations owing to fluctuations in circumstellar extinction at different characteristic times. The features of the photometric activity of the stars investigated are discussed in detail in this article.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Brightness</subject><subject>Clusters</subject><subject>Extinction</subject><subject>Light curve</subject><subject>Monitoring</subject><subject>Observations and Techniques</subject><subject>Photometry</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Star brightness</subject><subject>Stars</subject><subject>T Tauri stars</subject><subject>Variability</subject><issn>0571-7256</issn><issn>1573-8191</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp9kV1LIzEUhoOsYFf9A14F9mov4uajk2T2TsqqhS6KVvAuzGROaqQz6SYZqP_e1C5IYVkOnEB4nhxyXoQuGL1klKofidGKMUI5J7RWU0W2R2jCKiWIZjX7gia0UowoXskT9DWlV0ppLWs5QcunZ3wX53j5tgH8mJuYsB9wfgE8W48pQ8TzGRZT_RM_QBrXOeHg8CIMK7KE2OP7l5BDDzl6i3-HwecQ_bA6Q8euWSc4_3ueoqfrX8vZLVnc3cxnVwtiBWWZNFWrmbJdq7jSvJQQ9ZQpoVvnwDat1J3kjoHsWidrDVzKjipbVaAY1S0Tp-jb_t1NDH9GSNm8hjEOZaThSgihS5Of1KpZg_GDCzk2tvfJmivFtRS7kYW6_AdVqoPe2zCA8-X-QPh-IBQmwzavmjElM398OGT5nrUxpBTBmU30fRPfDKNmF6DZB2hKgOYjQLMtkthLabNbKsTP3_3HegcA5Znm</recordid><startdate>20220901</startdate><enddate>20220901</enddate><creator>Barsunova, O. Yu</creator><creator>Grinin, V. P.</creator><creator>Sergeev, S. G.</creator><creator>Shugarov, S. Yu</creator><creator>Efimova, N. V.</creator><creator>Nazarov, S. V.</creator><general>Springer US</general><general>Springer</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>ISR</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20220901</creationdate><title>UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring</title><author>Barsunova, O. Yu ; Grinin, V. P. ; Sergeev, S. G. ; Shugarov, S. Yu ; Efimova, N. V. ; Nazarov, S. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c301t-a5b817cdb7278282833941738bffecab68d62f1e6dbf698e266d07c55e7108b13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Brightness</topic><topic>Clusters</topic><topic>Extinction</topic><topic>Light curve</topic><topic>Monitoring</topic><topic>Observations and Techniques</topic><topic>Photometry</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Star brightness</topic><topic>Stars</topic><topic>T Tauri stars</topic><topic>Variability</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Barsunova, O. Yu</creatorcontrib><creatorcontrib>Grinin, V. P.</creatorcontrib><creatorcontrib>Sergeev, S. G.</creatorcontrib><creatorcontrib>Shugarov, S. Yu</creatorcontrib><creatorcontrib>Efimova, N. V.</creatorcontrib><creatorcontrib>Nazarov, S. V.</creatorcontrib><collection>CrossRef</collection><collection>Gale In Context: Science</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Astrophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Barsunova, O. Yu</au><au>Grinin, V. P.</au><au>Sergeev, S. G.</au><au>Shugarov, S. Yu</au><au>Efimova, N. V.</au><au>Nazarov, S. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring</atitle><jtitle>Astrophysics</jtitle><stitle>Astrophysics</stitle><date>2022-09-01</date><risdate>2022</risdate><volume>65</volume><issue>3</issue><spage>368</spage><epage>383</epage><pages>368-383</pages><issn>0571-7256</issn><eissn>1573-8191</eissn><abstract>Results of a long-term (17 years) photometric monitoring of five T Tau stars in the VRI bands are presented. All the studied objects are members of the young cluster IC 348 and show the UX Ori type variability caused by changes in the circumstellar extinction. Three of them (V712 Per, V716 Per, and V909 Per) are classical T Tau type stars (CTTS) and the other two (V695 Per, V715 Per) are weak-line T Tauri stars (WTTS). Their light curves demonstrate the large diversity. Three of the objects have a combination of two different types of activity: stochastic UX Ori type variability and periodic brightness variations similar to those observed in AA Tau stars. Two of the stars demonstrate only the stochastic brightness variations owing to fluctuations in circumstellar extinction at different characteristic times. The features of the photometric activity of the stars investigated are discussed in detail in this article.</abstract><cop>New York</cop><pub>Springer US</pub><doi>10.1007/s10511-022-09747-x</doi><tpages>16</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0571-7256 |
ispartof | Astrophysics, 2022-09, Vol.65 (3), p.368-383 |
issn | 0571-7256 1573-8191 |
language | eng |
recordid | cdi_proquest_journals_2733387336 |
source | Springer Nature |
subjects | Astronomy Astrophysics Astrophysics and Astroparticles Astrophysics and Cosmology Brightness Clusters Extinction Light curve Monitoring Observations and Techniques Photometry Physics Physics and Astronomy Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Star brightness Stars T Tauri stars Variability |
title | UX OrI Type Stars in the Cluster IC 348: Results of Long-Term Photometric Monitoring |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-30T22%3A11%3A15IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=UX%20OrI%20Type%20Stars%20in%20the%20Cluster%20IC%20348:%20Results%20of%20Long-Term%20Photometric%20Monitoring&rft.jtitle=Astrophysics&rft.au=Barsunova,%20O.%20Yu&rft.date=2022-09-01&rft.volume=65&rft.issue=3&rft.spage=368&rft.epage=383&rft.pages=368-383&rft.issn=0571-7256&rft.eissn=1573-8191&rft_id=info:doi/10.1007/s10511-022-09747-x&rft_dat=%3Cgale_proqu%3EA728631738%3C/gale_proqu%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c301t-a5b817cdb7278282833941738bffecab68d62f1e6dbf698e266d07c55e7108b13%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2733387336&rft_id=info:pmid/&rft_galeid=A728631738&rfr_iscdi=true |