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19952023
most citedA new chemo-evolutionary population synthesis model for early-type galaxies. I: Theoretical basis

393 citations · 2.7k across the 87 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 18 cited

Stellar Population Synthesis of star forming clumps in galaxy pairs and non-interacting spiral galaxies

Javier Zaragoza-Cardiel, Beverly J. Smith, Margarita Rosado +5

We have identified 1027 star forming complexes in a sample of 46 galaxies from the Spirals, Bridges, and Tails (SB&T) sample of interacting galaxies, and 693 star forming complexes…

astro-ph.HE2017★ 17 cited

Balmer filaments in Tycho's supernova remnant: an interplay between cosmic-ray and broad-neutral precursors

Sladjana Knežević, Ronald Läsker, Glenn van de Ven +8

We present H spectroscopic observations and detailed modelling of the Balmer filaments in the supernova remnant Tycho. We used Galaxy H Fabry-Pérot Spectrometer on the Willia…

astro-ph.HE2017

Balmer-dominated shocks in Tycho's SNR: omnipresence of CRs

Sladjana Knežević, Ronald Läsker, Glenn van de Ven +8

We present wide-field, spatially and highly resolved spectroscopic observations of Balmer filaments in the northeastern rim of Tycho's supernova remnant in order to investigate the…

astro-ph.GA2017★ 13 cited

Evolution of the anti-truncated stellar profiles of S0 galaxies since in the SHARDS survey: I - Sample and Methods

Alejandro Borlaff, M. Carmen Eliche-Moral, John E. Beckman +5

The controversy about the origin of the structure of S0--E/S0 galaxies may be due to the difficulty of comparing surface brightness profiles with different depths, photometric corr…

astro-ph.GA2017★ 9 cited

Physical properties of superbubbles in the Antennae galaxies

Artemi Camps-Fariña, Javier Zaragoza-Cardiel, John E. Beckman +4

Mass outflow generated by the dynamical feedback from massive stars is currently a topic of high interest. Using a purpose-developed analysis technique, and taking full advantage o…

astro-ph.GA2017★ 47 cited

Kinematic clues to bar evolution for galaxies in the local universe: why the fastest rotating bars are rotating most slowly

J. Font, J. E. Beckman, I. Martínez-Valpuesta +7

We have used Spitzer images of a sample of 68 barred spiral galaxies in the local universe to make systematic measurements of bar length and bar strength. We combine these with pre…