Actinium Abundance in the Atmospheres of Three Red Supergiants in the Magellanic Clouds
The actinium abundance in the atmospheres of red supergiants PMMR23 and PMMR144 in the Small Magellanic Cloud and RM_1-667 in the Large Magellanic Cloud was estimated. The results of spectral observations with the ESO 3.6-m telescope with resolving power R = 30000 were used. Since actinium was not f...
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| Veröffentlicht in: | Kinematics and physics of celestial bodies 2018-05, Vol.34 (3), p.123-133 |
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| container_title | Kinematics and physics of celestial bodies |
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| creator | Gopka, V. F. Shavrina, A. V. Yushchenko, V. A. Yushchenko, A. V. Pavlenko, Ya. V. Andrievsky, S. M. Vasileva, S. V. Kim, Ch Jeong, Y. Lyubchik, Yu. P. |
| description | The actinium abundance in the atmospheres of red supergiants PMMR23 and PMMR144 in the Small Magellanic Cloud and RM_1-667 in the Large Magellanic Cloud was estimated. The results of spectral observations with the ESO 3.6-m telescope with resolving power
R
= 30000 were used. Since actinium was not found in the atmospheres of PMMR23 and PMMR144, only the upper limits were set on its abundance: log
N
(Ac/H) |
| doi_str_mv | 10.3103/S0884591318030054 |
| format | Article |
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R
= 30000 were used. Since actinium was not found in the atmospheres of PMMR23 and PMMR144, only the upper limits were set on its abundance: log
N
(Ac/H) <–15.1 and–15.0, respectively. The estimated abundance of actinium in the atmosphere of RM_1-667 varied with parameters of the atmospheric model from–14.1 to–13.3. The lines of ionized actinium λ 616.475 nm and λ 581.085 nm were used in this analysis.</description><identifier>ISSN: 0884-5913</identifier><identifier>EISSN: 1934-8401</identifier><identifier>DOI: 10.3103/S0884591318030054</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Abundance ; Actinium ; Astronomy ; Atmosphere ; Atmospheres ; Atmospheric models ; European Southern Observatory ; Magellanic clouds ; Observations and Techniques ; Physics ; Physics and Astronomy ; Physics of Stars and Interstellar Medium ; Resolution</subject><ispartof>Kinematics and physics of celestial bodies, 2018-05, Vol.34 (3), p.123-133</ispartof><rights>Allerton Press, Inc. 2018</rights><rights>Kinematics and Physics of Celestial Bodies is a copyright of Springer, (2018). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-f05410cd08783561d55cb5d01bb4dcac8101c1d5d640b2dac1ee1711c7edff83</citedby><cites>FETCH-LOGICAL-c316t-f05410cd08783561d55cb5d01bb4dcac8101c1d5d640b2dac1ee1711c7edff83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.3103/S0884591318030054$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.3103/S0884591318030054$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Gopka, V. F.</creatorcontrib><creatorcontrib>Shavrina, A. V.</creatorcontrib><creatorcontrib>Yushchenko, V. A.</creatorcontrib><creatorcontrib>Yushchenko, A. V.</creatorcontrib><creatorcontrib>Pavlenko, Ya. V.</creatorcontrib><creatorcontrib>Andrievsky, S. M.</creatorcontrib><creatorcontrib>Vasileva, S. V.</creatorcontrib><creatorcontrib>Kim, Ch</creatorcontrib><creatorcontrib>Jeong, Y.</creatorcontrib><creatorcontrib>Lyubchik, Yu. P.</creatorcontrib><title>Actinium Abundance in the Atmospheres of Three Red Supergiants in the Magellanic Clouds</title><title>Kinematics and physics of celestial bodies</title><addtitle>Kinemat. Phys. Celest. Bodies</addtitle><description>The actinium abundance in the atmospheres of red supergiants PMMR23 and PMMR144 in the Small Magellanic Cloud and RM_1-667 in the Large Magellanic Cloud was estimated. The results of spectral observations with the ESO 3.6-m telescope with resolving power
R
= 30000 were used. Since actinium was not found in the atmospheres of PMMR23 and PMMR144, only the upper limits were set on its abundance: log
N
(Ac/H) <–15.1 and–15.0, respectively. The estimated abundance of actinium in the atmosphere of RM_1-667 varied with parameters of the atmospheric model from–14.1 to–13.3. The lines of ionized actinium λ 616.475 nm and λ 581.085 nm were used in this analysis.</description><subject>Abundance</subject><subject>Actinium</subject><subject>Astronomy</subject><subject>Atmosphere</subject><subject>Atmospheres</subject><subject>Atmospheric models</subject><subject>European Southern Observatory</subject><subject>Magellanic clouds</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Physics of Stars and Interstellar Medium</subject><subject>Resolution</subject><issn>0884-5913</issn><issn>1934-8401</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kE9Lw0AQxRdRsFY_gLcFz9GZbDbZHkPxH1QEG_AYNruTNiXdxN3k4Lc3pYoH8TQw7_feDI-xa4RbgSDu1qBUIhcoUIEAkMkJm-FCJJFKAE_Z7CBHB_2cXYSwm4g0XiQz9p6boXHNuOd5NTqrnSHeOD5siefDvgv9ljwF3tW82Hoi_kaWr8ee_KbRbgg_7IveUNtq1xi-bLvRhkt2Vus20NX3nLPi4b5YPkWr18fnZb6KjMB0iOrpUwRjQWVKyBStlKaSFrCqEmu0UQhopq1NE6hiqw0SYYZoMrJ1rcSc3Rxje999jBSGcteN3k0XyxikUioDGU8UHinjuxA81WXvm732nyVCeaiv_FPf5ImPnjCxbkP-N_l_0xdcFHEj</recordid><startdate>20180501</startdate><enddate>20180501</enddate><creator>Gopka, V. 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F.</au><au>Shavrina, A. V.</au><au>Yushchenko, V. A.</au><au>Yushchenko, A. V.</au><au>Pavlenko, Ya. V.</au><au>Andrievsky, S. M.</au><au>Vasileva, S. V.</au><au>Kim, Ch</au><au>Jeong, Y.</au><au>Lyubchik, Yu. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Actinium Abundance in the Atmospheres of Three Red Supergiants in the Magellanic Clouds</atitle><jtitle>Kinematics and physics of celestial bodies</jtitle><stitle>Kinemat. Phys. Celest. Bodies</stitle><date>2018-05-01</date><risdate>2018</risdate><volume>34</volume><issue>3</issue><spage>123</spage><epage>133</epage><pages>123-133</pages><issn>0884-5913</issn><eissn>1934-8401</eissn><abstract>The actinium abundance in the atmospheres of red supergiants PMMR23 and PMMR144 in the Small Magellanic Cloud and RM_1-667 in the Large Magellanic Cloud was estimated. The results of spectral observations with the ESO 3.6-m telescope with resolving power
R
= 30000 were used. Since actinium was not found in the atmospheres of PMMR23 and PMMR144, only the upper limits were set on its abundance: log
N
(Ac/H) <–15.1 and–15.0, respectively. The estimated abundance of actinium in the atmosphere of RM_1-667 varied with parameters of the atmospheric model from–14.1 to–13.3. The lines of ionized actinium λ 616.475 nm and λ 581.085 nm were used in this analysis.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.3103/S0884591318030054</doi><tpages>11</tpages></addata></record> |
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| subjects | Abundance Actinium Astronomy Atmosphere Atmospheres Atmospheric models European Southern Observatory Magellanic clouds Observations and Techniques Physics Physics and Astronomy Physics of Stars and Interstellar Medium Resolution |
| title | Actinium Abundance in the Atmospheres of Three Red Supergiants in the Magellanic Clouds |
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