skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Time monitoring of radio jets and magnetospheres in the nearby young stellar cluster R Coronae Australis

Journal Article · · Astrophysical Journal
; ; ; ; ;  [1]; ; ;  [2];  [3];  [4];  [5]
  1. Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei, 106, Taiwan (China)
  2. European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748, Garching (Germany)
  3. Department of Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180, Vienna (Austria)
  4. Centro de Radioastronomía y Astrofísica, UNAM, A.P. 3-72, Xangari, Morelia, 58089 (Mexico)
  5. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

We report Karl G. Jansky Very Large Array 8-10 GHz (λ = 3.0-3.7 cm) monitoring observations toward the young stellar object (YSO) cluster R Coronae Australis (R CrA), taken from 2012 March 15 to 2012 September 12. These observations were planned to measure the radio flux variabilities in timescales from 0.5 hr to several days, to tens of days, and up to ∼200 days. We found that among the YSOs detectable in individual epochs, in general, the most reddened objects in the Spitzer observations show the highest mean 3.5 cm Stokes I emission, and the lowest fractional variabilities on <200 day timescales. The brightest radio flux emitters in our observations are the two reddest sources IRS7W and IRS7E. In addition, by comparing our observations with observations taken from 1996 to 1998 and 2005, we found that the radio fluxes of these two sources have increased by a factor of ∼1.5. The mean 3.5 cm fluxes of the three Class I/II sources, IRSI, IRS2, and IRS6, appear to be correlated with their accretion rates derived by a previous near-infrared line survey. The weakly accreting Class I/II YSOs, or those in later evolutionary stages, present radio flux variability on <0.5 hr timescales. Some YSOs were detected only during occasional flaring events. The source R CrA went below our detection limit during a few fading events.

OSTI ID:
22348223
Journal Information:
Astrophysical Journal, Vol. 780, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

THE SPITZER SURVEY OF INTERSTELLAR CLOUDS IN THE GOULD BELT. III. A MULTI-WAVELENGTH VIEW OF CORONA AUSTRALIS
Journal Article · Wed Jun 01 00:00:00 EDT 2011 · Astrophysical Journal, Supplement Series · OSTI ID:22348223

Radio emission from pre-main-sequence stars in Corona Australis
Journal Article · Sun Nov 01 00:00:00 EST 1987 · Astrophys. J.; (United States) · OSTI ID:22348223

Very Large Array Multiband Monitoring Observations of M31*
Journal Article · Sun Aug 20 00:00:00 EDT 2017 · Astrophysical Journal · OSTI ID:22348223