activity
19952009
most citedAges and metallicities of early-type galaxies in the SDSS: new insight into the physical origin of the colour-magnitude and the Mg2-sigmaV relations

386 citations · 4.7k across the 101 of their papers we have counts for

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Showing 2009Show all

14 papers · 1 filter

astro-ph.HE2009

Constraining a possible time-variation of the gravitational constant through "gravitochemical heating" of neutron stars

Andreas Reisenegger, Paula Jofré, Rodrigo Fernández

A hypothetical time-variation of the gravitational constant would make neutron stars expand or contract, so the matter in their interiors would depart from beta equilibrium. Th…

astro-ph.SR20091 cited

Multi-wavelength observing of a forming solar-like star

S. G. Gregory, E. Flaccomio, C. Argiroffi +7

V2129 Oph is a 1.35 solar mass classical T Tauri star, known to possess a strong and complex magnetic field. By extrapolating from an observationally derived magnetic surface map,…

astro-ph.SR2009

Tepid Supergiants: Chemical Signatures of Stellar Evolution & The Extent of Blue Loops

Norbert Przybilla, Markus Firnstein, Maria-Fernanda Nieva

Massive stars can develop into tepid supergiants at several stages of their post main-sequence evolution, prior to core He-burning, on a blue loop, or close to the final supernova…

astro-ph.GA2009234 cited

Discrete sources as the origin of the Galactic X-ray ridge emission

Revnivtsev M., Sazonov S., Churazov E. +3

An unresolved X-ray glow (at energies above a few kiloelectronvolts) was discovered about 25 years ago and found to be coincident with the Galactic disk -the Galactic ridge X-ray e…

astro-ph.CO200925 cited

PHL 1092 as a transient extreme X-ray weak quasar

G. Miniutti, A. C. Fabian, W. N. Brandt +2

We report a dramatic variability event in the X-ray history of the Narrow-Line quasar PHL 1092 (z=0.396). Our latest 2008 XMM-Newton observation reveals a flux drop of ~200 with re…

astro-ph.IM2009

Using Virtual Observatory techniques to search for Adaptive Optics suitable AGN

J. Zuther, G. Lemson, A. Eckart +3

Until recently, it has been possible only for nearby galaxies to study the scaling relations between central black hole and host galaxy in detail. Because of the small number densi…