The supernova remnant population of the Small Magellanic Cloud

Pierre Maggi; Miroslav D. Filipović; Branislav Vukotić; Jean Ballet; Frank Haberl; Chandreyee Maitra; Patrick Kavanagh; Manami Sasaki; Milorad Stupar

doi:10.1051/0004-6361/201936583

Home

All issues

Volume 631 (November 2019)

A&A, 631 (2019) A127

Full HTML

Open Access

Fig. 2

Open with DEXTER Download original image

P × V^1∕2 of SNRs in SMC (orange triangles, this work) and LMC (grey plus signs, MHK16) as a function of their size. Lines of constant SN energy (times filling factor f, see text in Sect. 4.3.1) are overplotted in units of 10⁵¹ erg ≡1 foe.

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.