1995A&A...298..187B


Query : 1995A&A...298..187B

1995A&A...298..187B - Astronomy and Astrophysics, volume 298187-192 (1995/6-1)

VLBI observations of single main-sequence M stars.

BENZ A.O., ALEF W. and GUEDEL M.

Abstract (from CDS):

Single dMe stars have been observed at 18cm wavelength by intercontinental very long baseline interferometry (VLBI). Here we report on two stars, EQ Peg B and AD Leo, that have been detected during flares, and one of them also at a relatively low (`quiescent') state. There are no indications that any of the stars has been spatially resolved. Upper limits on the size of the radio sources are less than 1.9 stellar diameters for flares and less than 3.7 stellar diameters for quiescence. This yields directly observed brightness temperatures beyond 2x1010K for flares and 2x109K in quiescence. The observations suggest that the size of the closed corona is less than predicted from pressure equilibrium between plasma and magnetic field. An extent of the order of one density scale height is compatible with the observations.

Abstract Copyright: ∼

Journal keyword(s): stars: coronae - stars: flare - stars: late type - radio continuum: stars - techniques: interferometric

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
2 4C 15.05 Bla 02 04 50.41389294 +15 14 11.0436097   21.9 21.00 21.00   ~ 426 1
3 6C 073759+311929 Bla 07 41 10.70330407 +31 12 00.2291151   17.02 16.89 16.322   ~ 468 1
4 V* YZ CMi PM* 07 44 40.1723046464 +03 33 08.875227574 13.761 12.831 11.225 9.958 8.263 M4.0Ve 957 0
5 V* AD Leo PM* 10 19 36.2808181226 +19 52 12.010446571   10.82 9.52 9.19   dM3 1469 1
6 7C 1219+2830 BLL 12 21 31.6904439888 +28 13 58.500308172   16.81 16.11 14.24   ~ 924 1
7 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
8 BD+19 5116 ** 23 31 52.17898 +19 56 14.1505 12.737 11.749 10.165 8.982 7.446 M3.5V 469 0
9 BD+19 5116B PM* 23 31 52.5753377942 +19 56 14.005026315   14.8   12.165   M4.0Ve 222 0

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