Monthly Notices of the Royal Astronomical Society: Letters

Most Accessed

Enjoy these highly accessed papers recently published in the Monthly Notices of the Astronomical Society: LETTERS:

Cooling neutron star in the Cassiopeia A supernova remnant: evidence for superfluidity in the core, Vol 412:1

Discovery of a possibly old galaxy at z= 6.027, multiply imaged by the massive cluster Abell 383, Vol 414:1

Calibrating emission lines as quasar bolometers, Vol 412:1

Rotation of the Solar system planets and the origin of the Moon in the context of the tidal downsizing hypothesis, Vol 410:1

Detection of a planetary system orbiting the eclipsing polar HU Aqr, Vol 414:1

The 2010 nova outburst of the symbiotic Mira V407 Cyg, Vol 410:1

The distinction between star clusters and associations, Vol 410:1

The Subaru Lya blob survey: a sample of 100-kpc Lya blobs at z= 3?, Vol 410:1

The specific star formation rate of high redshift galaxies: the case for two modes of star formation, Vol 410:1

Too big to fail? The puzzling darkness of massive Milky Way subhaloes, Vol 415:1

The optimal weighting function for cosmic magnification measurements through the foreground galaxy–background galaxy (quasar) cross-correlation, Vol 415:1

The shortest period detached binary white dwarf system?, Vol 413:1

The causal connection between disc and power-law variability in hard state black hole X-ray binaries, Vol 414:1

Evidence for a black hole in the X-ray transient XTE J1859+226, Vol 413:1

Preparation of Kepler light curves for asteroseismic analyses, Vol 414:1

Ice chemistry in massive young stellar objects: the role of metallicity, Vol 411:1

Non-convergence of the critical cooling time-scale for fragmentation of self-gravitating discs, Vol 411:1

Bar fraction in lenticular galaxies: dependence on luminosity and environment, Vol 410:1

Prospects for detection of exoplanet magnetic fields through bow-shock observations during transits, Vol 411:1

How neutral is the intergalactic medium surrounding the redshift z = 7.085 quasar ULAS J1120+0641?, Vol 416:1