IAUC 4261 available at Central Bureau for Astronomical Telegrams.
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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4U 1820-30Morgan, E. H. et al.101986
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5-14 Μm Spitzer spectra of Themis family asteroids
We present 5-14 μm spectra of 8 Themis family asteroids observed with Spitzer. The diameter and geometric albedo are determined using the NEATM model. Their emissivity spectra is studied in order to determine if they exhibit an emission plateau at about 9 to 12 μm as observed in other primitive asteroids of the outer belt, attributed to fine
Alí-Lagoa, V. et al.Advertised on:
102011 -
A 3D extinction map of the northern Galactic plane based on IPHAS photometry
We present a 3D map of extinction in the northern Galactic plane derived using photometry from the INT/WFC Photometric Hα Survey of the northern Galactic plane. The map has fine angular ( ˜ 10 arcmin) and distance (100 pc) sampling allied to a significant depth (≳5 kpc). We construct the map using a method based on a hierarchical Bayesian model
Sale, S. E. et al.Advertised on:
102014 -
A catalog of observed nuclear magnitudes of Jupiter family comets
A catalog of a sample of 105 Jupiter family (JF) comets (defined as those with Tisserand constants T > 2 and orbital periods P < 20 yr) is presented with our ``best estimates'' of their absolute nuclear magnitudes H_N = V(1,0,0). The catalog includes all the nuclear magnitudes reported after 1950 until August 1998 that appear in the International
Tancredi, G. et al.Advertised on:
102000 -
A census of very-low-mass stars and brown dwarfs in the σ Orionis cluster
Context: The knowledge of the initial mass function (IMF) in open clusters constitutes one way of constraining the formation of low-mass stars and brown dwarfs, along with the frequency of multiple systems and the properties of disks. Aims: The aim of the project is to determine the shape of the mass function in the low-mass and substellar regimes
Lodieu, N. et al.Advertised on:
102009 -
A Cloud Model for the Upper Atmosphere of Jupiter
Not Available
Beckman, J. E.Advertised on:
101967