output
20002026
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations

Showing 2017Show all

19 papers · 1 filter

astro-ph.GA2017★ 7 cited

A deep narrowband survey for planetary nebulae at the outskirts of M33

R. Galera-Rosillo, R. L. M. Corradi, A. Mampaso

Context: Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect and explore the rich sy…

astro-ph.SR2017★ 25 cited

An UXor among FUors: extinction related brightness variations of the young eruptive star V582 Aur

P. Ábrahám, Á. Kóspál, M. Kun +24

V582 Aur is an FU Ori-type young eruptive star in outburst since 1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic va…

astro-ph.GA2017★ 17 cited

Chemical Abundances of Planetary Nebulae in the Substructures of M31 -- II. The Extended Sample and A Comparison Study with the Outer-disk Group

Xuan Fang, Ruben Garcia-Benito, Martin A. Guerrero +7

We report deep spectroscopy of ten planetary nebulae (PNe) in the Andromeda Galaxy (M31) using the 10.4m GTC. Our targets reside in different regions of M31, including halo streams…

astro-ph.SR2017★ 17 cited

The binary fraction of planetary nebula central stars: the promise of VPHAS+

Helen Barker, Albert Zijlstra, Orsola De Marco +5

The majority of planetary nebulae (PNe) are not spherical, and current single-star models cannot adequately explain all the morphologies we observe. This has led to the Binary Hypo…

astro-ph.GA2017★ 27 cited

A 100 kpc nebula associated with the "Teacup" fading quasar

Montserrat Villar Martin, Antonio Cabrera Lavers, Andrew Humphrey +4

We report the discovery of a ~100 kpc ionized nebula associated with the radio quiet type 2 quasar (QSO2) nicknamed the "Teacup" (z=0.085). The giant nebula is among the largest kn…

astro-ph.EP2017★ 32 cited

Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

A. Marciniak, P. Bartczak, T. Müller +40

The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a consequence of these select…