output
20022014
most citedThe James Webb Space Telescope

2k citations

Showing 2006Show all

42 papers · 1 filter

astro-ph200627 cited

Bulges and disks in the Host Galaxies of low redshift 3CR Sources: a near-IR view of their radial brightness profile

Carlos J. Donzelli, Marco Chiaberge, F. Duccio Macchetto +3

We analyze the near-infrared luminosity profiles and photometric parameters of the host galaxies of 3CR radio sources with z<0.3, to investigate their physical nature. Our sample i…

astro-ph200636 cited

Long-term infrared variability of the UX Ori-type star SV Cep

Attila Juhasz, Timo Prusti, Peter Abraham +1

We investigate the long-term optical-infrared variability of SV Cep, and explain it in the context of an existing UX Ori (UXOR) model. A 25-month monitoring programme was completed…

astro-ph200626 cited

NGC2298: a globular cluster on its way to disruption

Guido De Marchi, Luigi Pulone

We have studied the stellar main sequence (MS) of the globular cluster NGC2298 using deep HST/ACS observations in the F606W and F814W bands covering an area of 3.4' x 3.4' around t…

astro-ph200613 cited

Discovery of thirteen novae candidates in M87

Juan P. Madrid, William B. Sparks, Henry C. Ferguson +2

We have made thirteen positive identifications of near-ultraviolet (NUV) transient sources in the giant elliptical galaxy M87 using the Space Telescope Imaging Spectrograph (STIS)…

astro-ph2006276 cited

Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters

A. J. Cenarro, R. F. Peletier, P. Sanchez-Blazquez +7

We present a homogeneous set of stellar atmospheric parameters Teff, log g, [Fe/H] for MILES, a new spectral stellar library covering the range 3525 - 7500 angstrom at 2.3 angstrom…

astro-ph200666 cited

The onset of X-ray emission in young stellar objects: a Chandra observation of the Serpens star-forming region

G. Giardino, F. Favata, G. Micela +2

AIMS: To study the properties of X-ray emissions from young stellar objects (YSOs), through their evolution from Class I to Class III and determine whether Class 0 protostars emit…