University of Hertfordshire

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Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis. / Liu, Hauyu Baobab; Galván-Madrid, Roberto; Forbrich, Jan; Rodríguez, Luis F.; Takami, Michihiro; Costigan, Gráinne; Manara, Carlo Felice; Yan, Chi-Hung; Karr, Jennifer; Chou, Mei-Yin; Ho, Paul T. -P.; Zhang, Qizhou.

In: The Astrophysical Journal, Vol. 780, No. 2, 20.12.2013.

Research output: Contribution to journalArticlepeer-review

Harvard

Liu, HB, Galván-Madrid, R, Forbrich, J, Rodríguez, LF, Takami, M, Costigan, G, Manara, CF, Yan, C-H, Karr, J, Chou, M-Y, Ho, PT-P & Zhang, Q 2013, 'Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis', The Astrophysical Journal, vol. 780, no. 2. https://doi.org/10.1088/0004-637X/780/2/155

APA

Liu, H. B., Galván-Madrid, R., Forbrich, J., Rodríguez, L. F., Takami, M., Costigan, G., Manara, C. F., Yan, C-H., Karr, J., Chou, M-Y., Ho, P. T. -P., & Zhang, Q. (2013). Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis. The Astrophysical Journal, 780(2). https://doi.org/10.1088/0004-637X/780/2/155

Vancouver

Author

Liu, Hauyu Baobab ; Galván-Madrid, Roberto ; Forbrich, Jan ; Rodríguez, Luis F. ; Takami, Michihiro ; Costigan, Gráinne ; Manara, Carlo Felice ; Yan, Chi-Hung ; Karr, Jennifer ; Chou, Mei-Yin ; Ho, Paul T. -P. ; Zhang, Qizhou. / Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis. In: The Astrophysical Journal. 2013 ; Vol. 780, No. 2.

Bibtex

@article{493cf194a42f45bdbd4d9ea400589372,
title = "Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis",
abstract = "We report JVLA 8-10 GHz ($\lambda$=3.0-3.7 cm) monitoring observations toward the YSO cluster R Coronae Australis (R\,CrA), taken in 2012, from March 15 to September 12. These observations were planned to measure the radio flux variabilities in timescales from 0.5 hours to several days, to tens of days, and up to $\sim$200 days. We found that among the YSOs detectable in individual epochs, in general, the most reddened objects in the \textit{Spitzer} observations show the highest mean 3.5 cm Stokes \textit{I} emission, and the lowest fractional variabilities on $ $",
keywords = "astro-ph.SR",
author = "Liu, {Hauyu Baobab} and Roberto Galv{\'a}n-Madrid and Jan Forbrich and Rodr{\'i}guez, {Luis F.} and Michihiro Takami and Gr{\'a}inne Costigan and Manara, {Carlo Felice} and Chi-Hung Yan and Jennifer Karr and Mei-Yin Chou and Ho, {Paul T. -P.} and Qizhou Zhang",
note = "Accepted to ApJ",
year = "2013",
month = dec,
day = "20",
doi = "10.1088/0004-637X/780/2/155",
language = "English",
volume = "780",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "2",

}

RIS

TY - JOUR

T1 - Time Monitoring of Radio Jets and Magnetospheres in the Nearby Young Stellar Cluster R Coronae Australis

AU - Liu, Hauyu Baobab

AU - Galván-Madrid, Roberto

AU - Forbrich, Jan

AU - Rodríguez, Luis F.

AU - Takami, Michihiro

AU - Costigan, Gráinne

AU - Manara, Carlo Felice

AU - Yan, Chi-Hung

AU - Karr, Jennifer

AU - Chou, Mei-Yin

AU - Ho, Paul T. -P.

AU - Zhang, Qizhou

N1 - Accepted to ApJ

PY - 2013/12/20

Y1 - 2013/12/20

N2 - We report JVLA 8-10 GHz ($\lambda$=3.0-3.7 cm) monitoring observations toward the YSO cluster R Coronae Australis (R\,CrA), taken in 2012, from March 15 to September 12. These observations were planned to measure the radio flux variabilities in timescales from 0.5 hours to several days, to tens of days, and up to $\sim$200 days. We found that among the YSOs detectable in individual epochs, in general, the most reddened objects in the \textit{Spitzer} observations show the highest mean 3.5 cm Stokes \textit{I} emission, and the lowest fractional variabilities on $ $

AB - We report JVLA 8-10 GHz ($\lambda$=3.0-3.7 cm) monitoring observations toward the YSO cluster R Coronae Australis (R\,CrA), taken in 2012, from March 15 to September 12. These observations were planned to measure the radio flux variabilities in timescales from 0.5 hours to several days, to tens of days, and up to $\sim$200 days. We found that among the YSOs detectable in individual epochs, in general, the most reddened objects in the \textit{Spitzer} observations show the highest mean 3.5 cm Stokes \textit{I} emission, and the lowest fractional variabilities on $ $

KW - astro-ph.SR

U2 - 10.1088/0004-637X/780/2/155

DO - 10.1088/0004-637X/780/2/155

M3 - Article

VL - 780

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

ER -