Highlight
Free Access

Table 5

The quantity and mass of H2O maser clouds.

Star Epochs tall ni nq/ni tcross Ntot Mcloud clouds fV ns/n
(yr) (m-3) (yr) P (M) (M yr-1)

VX Sgr 94–99 4.73 4.7 × 1013 107 89 139* 3 1.1 × 10-5 1.7 × 10-5 0.2 0.0009 0.90
S Per 94–99 4.80 1.2 × 1014 43 38 134* 6 1.4 × 10-5 4.8 × 10-5 1.3 0.0095 0.60
U Ori 99–00–01 2.30 6.9 × 1013 72 32 57 2 2.4 × 10-7 4.2 × 10-7 1.8 0.0095 0.31
U Her 00–01 0.94 5.7 × 1013 88 29 62 2 2.9 × 10-7 6.1 × 10-7 1.8 0.0079 0.31
IK Tau 00–01 0.94 6.7 × 1013 75 24 85 4 1.6 × 10-7 5.4 × 10-7 0.2 0.0010 0.92
RT Vir 96(6) 0.186 9.2 × 1013 55 11 142 6 3.8 × 10-9 5.1 × 10-8 0.4 0.0026 0.86
W Hya 99–00–01–02 3.16 9.1 × 1013 55 14 45 3 1.5 × 10-8 5.1 × 10-8 0.2 0.0019 0.90

Notes. tall is the timespan covered by the epochs used in this analysis. ni is the number density at ri estimated from mass loss rates taken from the literature (Table 1) and nq/ni is the ratio of the quenching density to ni. tcross is the estimated crossing time for the 22-GHz maser shell. Ntot and Ntot/P are the total number of maser clouds at any one time and the number produced per stellar period, respectively. The mass per H2O maser cloud is Mcloud, clouds is the mass loss rate in clouds and clouds/ is the ratio of this to the mass loss rate from the literature. fV is the volume filling factor of the clouds in the shell. ns/n is the fractional number density of the wind surrounding the clouds.

(*)

The actual number of clouds may be less since some RSG clouds are large enough to contain several features.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.