Free Access

Table 16

3σ upper limits for the absorption-corrected luminosities for Nova M31N 1997-10c.

Observation LX/1037 erg s-1 (0.2–1.0 keV)

c2 10.8+
c3 1.9
c4 1.0



The count rate detected in observation c2 gives a luminosity of 2.4  ±  2.8  ×  1037 erg s-1, which results in the upper limit given in the Table. The fact that this upper limit is higher than the luminosity detected in observation c1 is, at least in part, attributed to the very short effective observing time of less than 6000 s.

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.