activity
20052009
most citedBiases on initial mass function determinations. III. Cluster masses derived from unresolved photometry

41 citations · 84 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM200941 cited

Biases on initial mass function determinations. III. Cluster masses derived from unresolved photometry

J. Maíz Apellániz

It is currently common to use spatially unresolved multi-filter broad-band photometry to determine the masses of individual stellar clusters (and hence the cluster mass function, C…

astro-ph2008

Spectroscopic monitoring of Southern Galactic O and WN stars: State of the Art in 2007

R. Gamen, R. Barba, N. Morrell +5

We are conducting a spectroscopic monitoring of O and WN -type stars in our Galaxy. In this work, we summarize some of our first results related to the search for radial-velocity v…

astro-ph200736 cited

Testing the predicted mass-loss bi-stability jump at radio wavelengths

P. Benaglia, J. S. Vink, J. Marti +3

In this study, we test the theoretically predicted mass-loss behaviour as a function of stellar effective temperature across the so-called `bi-stability' jump (BSJ). We gathered ra…

astro-ph20067 cited

A uniform set of optical/NIR photometric zero points to be used with CHORIZOS

J. Maíz Apellániz

I have recently combined HST/STIS spectrophotometry with existing photometric data to analyze the calibration of three standard optical photometry systems: Tycho-2 B_TV_T, Stromgre…

astro-ph2005

The infrared Hourglass cluster in M8

J. Arias, R. Barba, J. Maiz Apellaniz +2

A detailed study of the Hourglass Nebula in the M8 star forming region is presented. The study is mainly based on recent subarcsec-resolution JHKs images taken at Las Campanas Obse…

astro-ph2005

Deriving stellar properties from photometry: maximizing information content and minimizing biases

J. Maíz Apellániz

I study the importance of the accurate calibration of photometric systems in order to produce meaningful comparisons between the observed colors + magnitudes and model SEDs. Possib…