Evolved star water maser cloud size determined by star size

Free Access

Table 4

Continued. A shift V_corr applied to the Pushchino data, see Figs. 42 to 43.

Source	Date	V_LSR	Peak	I_tot
Telescope	(YYMMDD)	(km s^-1)	(Jy)	(Jy km s^-1)

W Hya
Pushchino	990119	39.9	128.6	245
MERLIN	990209	39.8	91.0	177
Pushchino	990310	39.8	174.7	323

Pushchino	000331	40.4	81.4	176
MERLIN	000405	40.6	59.2	169¹
Pushchino	000425	40.4	169.8	304

Pushchino	010411	40.4	377.3	413
MERLIN	010430	40.4	163.8	204
Pushchino	010904	40.3	554.8	471

Pushchino	020326	40.2	690.8	917
MERLIN	020405	40.2	296.9	335
Pushchino	020422	40.2	202.5	255

Notes. No emission above 10 Jy was detected by Pushchino at the adjacent epochs around this velocity. The integrated MERLIN flux density excluding this feature is 106 Jy km s^-1.

⁽¹⁾

At this epoch, a peak of 90.8 Jy was seen in the MERLIN W Hya spectrum at 44.7 km s^-1.

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.