2026ApJ...998..113W


Query : 2026ApJ...998..113W

2026ApJ...998..113W - Astrophys. J., 998, 113 (2026/February-2)

HST Observations of HD 166620 and τ Ceti: First UV Spectra of a Magnetic Grand Minimum Star and the Extent of τ Ceti's Astrosphere.

WOOD B.E., MULLER H.-R., HARTSHORN D., REDFIELD S. and METCALFE T.S.

Abstract (from CDS):

We present new Hubble Space Telescope (HST) UV spectra of the K2 V star HD 166620, the first star clearly recognized to be in a “magnetic grand minimum” state analogous to the Sun's “Maunder minimum” in the late 1600s. The stellar H I Lyα surface fluxes are extremely low, about a factor of 2 below fluxes observed during solar minimum, and also significantly lower than those of τ Ceti (G8 V) and HD 191408 (K2.5 V), two stars more similar to HD 166620 in spectral type and age (∼10 Gyr) than the Sun. The τ Ceti data that are compared with HD 166620 include both old archival data and a new HST observation as well. The Lyα data are used to confirm a nondetection of astrospheric Lyα absorption for this star, suggesting a very weak wind with $\dot{M}\lt 0.1$${\dot{M}}_{\odot }$. The very compact astrosphere inferred for τ Ceti indicates that the star's debris disk is at least partly exposed to the interstellar medium (ISM), and we discuss possible consequences.

Abstract Copyright: © 2026. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Interstellar absorption - Ultraviolet spectroscopy - Stellar chromospheres - Debris disks - Stellar winds - Interstellar medium - Stellar-interstellar interactions

Simbad objects: 17

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Number of rows : 17
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 * tau Cet PM* 01 44 04.0831371922 -15 56 14.927607677 4.43 4.22 3.50 2.88 2.41 G8V 1354 1
2 HD 15115 PM* 02 26 16.2457848552 +06 17 33.186453252   7.15 6.80   6.33 F4IV 225 0
3 NAME G Cloud Cld 03 00 +50.2           ~ 85 0
4 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 2073 1
5 NAME LIC Cld 04 41 +31.           ~ 317 0
6 HD 32297 * 05 02 27.4358754192 +07 27 39.678553260   8.32 8.14     A0V 234 0
7 * bet Pic PM* 05 47 17.0876901 -51 03 59.441135 4.13 4.03 3.86 3.74 3.58 A6V 2087 1
8 HD 61005 PM* 07 35 47.4623556456 -32 12 14.045086368   8.96 8.22     G8Vk 265 0
9 * 61 Vir PM* 13 18 24.3139864471 -18 18 40.297748582 5.710 5.440 4.740     G6.5V 742 1
10 * ksi Boo BY* 14 51 23.37993 +19 06 01.6994 5.618 5.370 4.593 3.91 3.48 G7Ve+K5Ve 503 0
11 HD 166620 PM* 18 09 37.4162111401 +38 27 27.998016381 7.86 7.27 6.40 5.63 5.14 K2V 481 0
12 NAME Mic Cloud Cld 18 10 +13.           ~ 15 0
13 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
14 BD+41 3306 PM* 19 19 00.5489000285 +41 38 04.582441681 10.01 9.67 8.86 8.18 7.66 K0V 331 0
15 HD 191408 PM* 20 11 11.9387690214 -36 06 04.351725607   5.44 5.32     K2.5V 294 1
16 Ross 825 ** 21 11 17.05579 +33 31 27.2904   12.421 11.462 11.125   K3 33 0
17 NAME Local Bubble ISM ~ ~           ~ 1059 0

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