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 2007 · astro-phShow all

27 papers · 2 filters

astro-ph200768 cited

The dark matter halo of NGC 1399 - CDM or MOND?

T. Richtler, Y. Schuberth, M. Hilker +3

Central galaxies in galaxy clusters may be key discriminants in the competition between the cold dark matter (CDM) paradigm and modified Newtonian dynamics (MOND). We investigate t…

astro-ph200766 cited

The impact of Spitzer infrared data on stellar mass estimates - and a revised galaxy stellar mass function at 0 < z < 5

F. Elsner, G. Feulner, U. Hopp

Aims: We estimate stellar masses of galaxies in the high redshift universe with the intention of determining the influence of newly available Spitzer/IRAC infrared data on the anal…

astro-ph20079 cited

High-Mass X-ray Binaries and the Spiral Structure of the Host Galaxy

P. Shtykovskiy, M. Gilfanov

We investigate the manifestation of the spiral structure in the distribution of high-mass X-ray binaries (HMXBs) over the host galaxy. We construct the simple kinematic model. It s…

astro-ph200740 cited

Intra Cluster Globular Clusters around NGC 1399 in Fornax?

Y. Schuberth, T. Richtler, L. Bassino +1

We investigate whether the globular clusters (GCs) in the recently published sample of GCs in the Fornax cluster by Bergond and coworkers are indeed intra-cluster objects. We combi…

astro-ph200730 cited

High Mass X-ray Binaries and Recent Star Formation History of the Small Magellanic Cloud

P. Shtykovskiy, M. Gilfanov

We study the relation between high-mass X-ray binary (HMXB) population and recent star formation history (SFH) for the Small Magellanic Cloud (SMC). Using archival optical SMC obse…

astro-ph200728 cited

Ejecta and progenitor of the low-luminosity Type IIP supernova 2003Z

V. P. Utrobin, N. N. Chugai, A. Pastorello

The origin of low-luminosity Type IIP supernovae is unclear: they have been proposed to originate either from massive (about 25 Msun) or low-mass (about 9 Msun) stars. We wish to d…