Jupiter analogues and planets of active stars

Combined results are now available from a 15 year long search for Jupiter analogues around solar-type stars using the ESO CAT + CES, ESO 3.6 m + CES, and ESO 3.6 m + HARPS instruments. They comprise planet (co-)discoveries (ι Hor and HR 506) and confirmations (three planets in HR 3259) as well as no...
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Autor*in:	Henning T. [verfasserIn] Nilsson H. [verfasserIn] Hartman H. [verfasserIn] Lo Curto G. [verfasserIn] Endl M. [verfasserIn] Zechmeister M. [verfasserIn] Kürster M. [verfasserIn] Hatzes A.P. [verfasserIn] Cochran W.D. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2013

Übergeordnetes Werk:	In: EPJ Web of Conferences - EDP Sciences, 2010, 47, p 05005(2013)
Übergeordnetes Werk:	volume:47, p 05005 ; year:2013

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1051/epjconf/20134705005

Katalog-ID:	DOAJ067276636

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allfieldsSound	10.1051/epjconf/20134705005 doi (DE-627)DOAJ067276636 (DE-599)DOAJccd7217faf5a4a8fbf6380f01881e702 DE-627 ger DE-627 rakwb eng QC1-999 Henning T. verfasserin aut Jupiter analogues and planets of active stars 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Combined results are now available from a 15 year long search for Jupiter analogues around solar-type stars using the ESO CAT + CES, ESO 3.6 m + CES, and ESO 3.6 m + HARPS instruments. They comprise planet (co-)discoveries (ι Hor and HR 506) and confirmations (three planets in HR 3259) as well as non-confirmations of planets (HR 4523 and ɛ Eri) announced elsewhere. A long-term trend in ɛ Ind found by our survey is probably attributable to a Jovian planet with a period <30 yr, but we cannot fully exclude stellar activity effects as the cause. A 3.8 year periodic variation in HR 8323 can be attributed to stellar activity. Physics Nilsson H. verfasserin aut Hartman H. verfasserin aut Lo Curto G. verfasserin aut Endl M. verfasserin aut Zechmeister M. verfasserin aut Kürster M. verfasserin aut Hatzes A.P. verfasserin aut Cochran W.D. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 47, p 05005(2013) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:47, p 05005 year:2013 https://doi.org/10.1051/epjconf/20134705005 kostenfrei https://doaj.org/article/ccd7217faf5a4a8fbf6380f01881e702 kostenfrei http://dx.doi.org/10.1051/epjconf/20134705005 kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 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_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 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 47, p 05005 2013
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authorswithroles_txt_mv	Henning T. @@aut@@ Nilsson H. @@aut@@ Hartman H. @@aut@@ Lo Curto G. @@aut@@ Endl M. @@aut@@ Zechmeister M. @@aut@@ Kürster M. @@aut@@ Hatzes A.P. @@aut@@ Cochran W.D. @@aut@@
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title	Jupiter analogues and planets of active stars
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title_auth	Jupiter analogues and planets of active stars
abstract	Combined results are now available from a 15 year long search for Jupiter analogues around solar-type stars using the ESO CAT + CES, ESO 3.6 m + CES, and ESO 3.6 m + HARPS instruments. They comprise planet (co-)discoveries (ι Hor and HR 506) and confirmations (three planets in HR 3259) as well as non-confirmations of planets (HR 4523 and ɛ Eri) announced elsewhere. A long-term trend in ɛ Ind found by our survey is probably attributable to a Jovian planet with a period <30 yr, but we cannot fully exclude stellar activity effects as the cause. A 3.8 year periodic variation in HR 8323 can be attributed to stellar activity.
abstractGer	Combined results are now available from a 15 year long search for Jupiter analogues around solar-type stars using the ESO CAT + CES, ESO 3.6 m + CES, and ESO 3.6 m + HARPS instruments. They comprise planet (co-)discoveries (ι Hor and HR 506) and confirmations (three planets in HR 3259) as well as non-confirmations of planets (HR 4523 and ɛ Eri) announced elsewhere. A long-term trend in ɛ Ind found by our survey is probably attributable to a Jovian planet with a period <30 yr, but we cannot fully exclude stellar activity effects as the cause. A 3.8 year periodic variation in HR 8323 can be attributed to stellar activity.
abstract_unstemmed	Combined results are now available from a 15 year long search for Jupiter analogues around solar-type stars using the ESO CAT + CES, ESO 3.6 m + CES, and ESO 3.6 m + HARPS instruments. They comprise planet (co-)discoveries (ι Hor and HR 506) and confirmations (three planets in HR 3259) as well as non-confirmations of planets (HR 4523 and ɛ Eri) announced elsewhere. A long-term trend in ɛ Ind found by our survey is probably attributable to a Jovian planet with a period <30 yr, but we cannot fully exclude stellar activity effects as the cause. A 3.8 year periodic variation in HR 8323 can be attributed to stellar activity.
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title_short	Jupiter analogues and planets of active stars
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