VLBI observations of a strong radio flare in HR 1099

Details VLBI observations of a strong radio flare in HR 1099 VLBI observations of a strong radio flare in HR 1099

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..903t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 4, p. 903-907.

Astronomy and Astrophysics

Astronomy

26

Radio Stars, Stellar Flares, Very Long Base Interferometry, Binary Stars, Radio Emission

Scientific paper

In 1991 July, we studied a strong radio flare in the RS CVn system HR 1099 with VLBI techniques. This system is one in a list of stars which we regularly monitor with the Noto 32-m antenna at 6 cm. The angular size of the radio source was found to increase at the beginning of the flare. It reached about 4 mas, which corresponds to a linear size comparable to that of the entire binary system. An upper limit of 80 G for the magnetic field was derived. The flare decay reflects the change of the power spectrum of the emitting electrons towards lower energies, due to radiative losses and interaction with the local plasma.

Affiliated with

Also associated with

No associations

Rating

VLBI observations of a strong radio flare in HR 1099 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with VLBI observations of a strong radio flare in HR 1099, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBI observations of a strong radio flare in HR 1099 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1276011