Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ ZENODOarrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Conference object . 2016
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Other literature type . 2016
License: CC BY
Data sources: ZENODO
versions View all 1 versions
addClaim

Evidence For A Double Coronal Cycle In The Young Solar Analog Iota Hor

Authors: Sanz-Forcada, Jorge; Stelzer, Beate;

Evidence For A Double Coronal Cycle In The Young Solar Analog Iota Hor

Abstract

Activity cycles are commonly found among late type stars through the chromospheric Ca II emission. Their coronal counterpart, however, remains elusive in most cases, despite of the clear X-ray cycle observed in the solar corona, spanning as much as 1.7 dex in L x . The recent discovery of a Ca II cycle in iota Hor of just 1.6 yr, the shortest to date, offered us a unique opportunity to monitor its X-ray counterpart in short time. The star offers also two more interesting properties: a planet of ~1.9 MJ orbits the star at 0.9 a.u., and with an age of only ~600 Myr and spectral type F8V, ι Hor represents a young solar analog, so its cycle might be the paradigm of the first activity cycles in the life of a solar-like star. Our XMM-Newton observations show the first coronal cycle in a single star. In good agreement with Ca II contemporaneous observations, the long term XMM-Newton light curve suggests also a long-term trend that seems to modulate the 1.6 yr cycle. Iota Hor may offer us the unique possibility to observe for the first time a double coronal cycle similar to those observed in the chromosphere of other stars.

{"references": ["Ayres, T. R. 2009, ApJ, 696, 1931", "Ayres, T. R. 2014, AJ, 147, 59", "B\u00f6hm-Vitense, E. 2007, ApJ, 657, 486", "Favata, F., Micela, G., Baliunas, S. L., et al. 2004, A&A, 418, L13", "Favata, F., Micela, G., Orlando, S., et al. 2008, A&A, 490, 1121", "G\u00fcdel, M. 2004, A&ARv, 12, 71", "Hempelmann, A., Robrade, J., Schmitt, J. H. M. M., et al. 2006, A&A, 460, 261", "Judge, P. G., Solomon, S. C., & Ayres, T. R. 2003, ApJ, 593, 534", "Lalitha, S.; Schmitt, J. H. M. M. 2013, A&A, 559, 119", "Lorente, R., & Montesinos, B. 2005, ApJ, 632, 1104", "Metcalfe, T. S., Basu, S., Henry, T. J., et al. 2010, ApJ, 723, L213", "Orlando, S., Peres, G., & Reale, F. 2001, ApJ, 560, 499", "Robrade, J., Schmitt, J. H. M. M., & Favata, F. 2005, A&A, 442, 315", "Robrade, J., Schmitt, J. H. M. M., & Favata, F. 2012, A&A, 543, A84", "Sanz-Forcada, J.; Maggio, A.; Micela, G. 2003, A&A, 408, 1087", "Sanz-Forcada, J.; Stelzer, B.; Metcalfe, T. S. 2013, A&A, 553, L6"]}

Poster #227

Keywords

astrobiology, activity cycles, stellar coronae, planetary systems

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    0
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
    OpenAIRE UsageCounts
    Usage byUsageCounts
    visibility views 3
    download downloads 6
  • 3
    views
    6
    downloads
    Powered byOpenAIRE UsageCounts
Powered by OpenAIRE graph
Found an issue? Give us feedback
visibility
download
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
OpenAIRE UsageCountsViews provided by UsageCounts
downloads
OpenAIRE UsageCountsDownloads provided by UsageCounts
0
Average
Average
Average
3
6
Green