output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2019 · astro-ph.SRShow all

33 papers · 2 filters

astro-ph.SR2019★ 35 cited

Pulsation in faint blue stars

Conor M. Byrne, C. Simon Jeffery

Following the discovery of blue large-amplitude pulsators (BLAPs) by the OGLE survey, additional hot, high-amplitude pulsating stars have been discovered by the Zwicky Transient Fa…

astro-ph.SR2019★ 10 cited

The circumstellar environment of 55 Cnc: The super-Earth 55 Cnc e as a primary target for star-planet interactions

C. P. Folsom, D. Ó Fionnagáin, L. Fossati +5

Context. 55 Cancri hosts five known exoplanets, most notably the hot super-Earth 55 Cnc e, which is one of the hottest known transiting super-Earths. Aims. Due to the short orbital…

astro-ph.SR2019★ 35 cited

Evolution of the Alfvén Mach number associated with a coronal mass ejection shock

Ciara A. Maguire, Eoin P. Carley, Joseph McCauley +1

The Sun regularly produces large-scale eruptive events, such as coronal mass ejections (CMEs) that can drive shock waves through the solar corona. Such shocks can result in electro…

astro-ph.SR2019★ 7 cited

Massive black holes regulated by luminous blue variable mass loss and magnetic fields

Jose H. Groh, Eoin Farrell, Georges Meynet +5

We investigate the effects of mass loss during the main-sequence (MS) and post-MS phases of massive star evolution on black hole (BH) birth masses. We compute solar metallicity Gen…

astro-ph.SR2019★ 4 cited

Different types of star-planet interactions

A. A. Vidotto

Stars and their exoplanets evolve together. Depending on the physical characteristics of these systems, such as age, orbital distance and activity of the host stars, certain types…

astro-ph.SR2019★ 9 cited

Stellar cosmic rays as an important source of ionisation in protoplanetary disks: a disk mass dependent process

D. Rodgers-Lee, A. M. Taylor, T. P. Downes +1

We assess the ionising effect of low energy protostellar cosmic rays in protoplanetary disks around a young solar mass star for a wide range of disk parameters. We assume a source…