Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves

To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 years including recent observations of ISO and Spitzer....
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Young-Joo Kwon [verfasserIn] Kyung-Won Suh [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2010

Schlagwörter:	stars: asymptotic giant branch and post-asymptotic giant branch infrared: stars stars: oscillations circumstellar matter dust: extinction

Übergeordnetes Werk:	In: Journal of Astronomy and Space Sciences - Korean Space Science Society (KSSS), 2012, 27(2010), 4, Seite 279-288
Übergeordnetes Werk:	volume:27 ; year:2010 ; number:4 ; pages:279-288

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.5140/JASS.2010.27.4.279

Katalog-ID:	DOAJ066715849

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allfieldsSound	10.5140/JASS.2010.27.4.279 doi (DE-627)DOAJ066715849 (DE-599)DOAJb947ff4caa134f4298e93046940998a4 DE-627 ger DE-627 rakwb eng QB1-991 Young-Joo Kwon verfasserin aut Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 years including recent observations of ISO and Spitzer. We use Marquardt-Levenberg algorithm to determine the pulsation periods and amplitudes and compare them with previous results of infrared and radio investigations. Generally, the newly determined pulsation parameters show much less errors because of the larger database. We find that the relationship between the pulsation period and amplitudes at M band is fairly well fitted with a simple linear equation in a wide period range. For OH 42.3-0.1, we find some evidences that the object could be a post-asymptotic giant branch star. stars: asymptotic giant branch and post-asymptotic giant branch infrared: stars stars: oscillations circumstellar matter dust: extinction Astronomy Kyung-Won Suh verfasserin aut In Journal of Astronomy and Space Sciences Korean Space Science Society (KSSS), 2012 27(2010), 4, Seite 279-288 (DE-627)62761471X (DE-600)2557343-3 20931409 nnns volume:27 year:2010 number:4 pages:279-288 https://doi.org/10.5140/JASS.2010.27.4.279 kostenfrei https://doaj.org/article/b947ff4caa134f4298e93046940998a4 kostenfrei http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2010/v27n4/OJOOBS_2010_v27n4_279.pdf kostenfrei https://doaj.org/toc/2093-5587 Journal toc kostenfrei https://doaj.org/toc/2093-1409 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 27 2010 4 279-288
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source	In Journal of Astronomy and Space Sciences 27(2010), 4, Seite 279-288 volume:27 year:2010 number:4 pages:279-288
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topic_facet	stars: asymptotic giant branch and post-asymptotic giant branch infrared: stars stars: oscillations circumstellar matter dust: extinction Astronomy
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authorswithroles_txt_mv	Young-Joo Kwon @@aut@@ Kyung-Won Suh @@aut@@
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spellingShingle	Young-Joo Kwon misc QB1-991 misc stars: asymptotic giant branch and post-asymptotic giant branch misc infrared: stars misc stars: oscillations misc circumstellar matter misc dust: extinction misc Astronomy Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves
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topic_title	QB1-991 Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves stars: asymptotic giant branch and post-asymptotic giant branch infrared: stars stars: oscillations circumstellar matter dust: extinction
topic	misc QB1-991 misc stars: asymptotic giant branch and post-asymptotic giant branch misc infrared: stars misc stars: oscillations misc circumstellar matter misc dust: extinction misc Astronomy
topic_unstemmed	misc QB1-991 misc stars: asymptotic giant branch and post-asymptotic giant branch misc infrared: stars misc stars: oscillations misc circumstellar matter misc dust: extinction misc Astronomy
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title	Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves
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title_sort	properties of the variation of the infrared emission of oh/ir stars iii. the m band light curves
callnumber	QB1-991
title_auth	Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves
abstract	To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 years including recent observations of ISO and Spitzer. We use Marquardt-Levenberg algorithm to determine the pulsation periods and amplitudes and compare them with previous results of infrared and radio investigations. Generally, the newly determined pulsation parameters show much less errors because of the larger database. We find that the relationship between the pulsation period and amplitudes at M band is fairly well fitted with a simple linear equation in a wide period range. For OH 42.3-0.1, we find some evidences that the object could be a post-asymptotic giant branch star.
abstractGer	To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 years including recent observations of ISO and Spitzer. We use Marquardt-Levenberg algorithm to determine the pulsation periods and amplitudes and compare them with previous results of infrared and radio investigations. Generally, the newly determined pulsation parameters show much less errors because of the larger database. We find that the relationship between the pulsation period and amplitudes at M band is fairly well fitted with a simple linear equation in a wide period range. For OH 42.3-0.1, we find some evidences that the object could be a post-asymptotic giant branch star.
abstract_unstemmed	To study properties of the pulsation in the infrared emission for long period variables, we have collected and analyzed the infrared observational data at M band for 12 OH/IR stars. We present the light curves using the data that cover about 30 years including recent observations of ISO and Spitzer. We use Marquardt-Levenberg algorithm to determine the pulsation periods and amplitudes and compare them with previous results of infrared and radio investigations. Generally, the newly determined pulsation parameters show much less errors because of the larger database. We find that the relationship between the pulsation period and amplitudes at M band is fairly well fitted with a simple linear equation in a wide period range. For OH 42.3-0.1, we find some evidences that the object could be a post-asymptotic giant branch star.
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title_short	Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves
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Properties of the Variation of the Infrared Emission of OH/IR Stars III. The M Band Light Curves

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