We generalize the technique of Lada et al.([CITE]) to map dust column density through a
molecular cloud (Nice) to an optimized multi-band technique (Nicer) that can be applied to …

This paper presents large scale extinction maps of most nearby Giant Molecular Clouds of
the Galaxy (Lupus, rho-Ophiuchus, Scorpius, Coalsack, Taurus, Chamaeleon, Musca …

We present a new catalog of 108 Herbig Ae/Be candidate stars identified in the Pico dos
Dias Survey, together with 19 previously known candidates and four objects selected from …

Herschel has shown that filamentary structures are ubiquitous in star-forming regions, in
particular in nearby molecular clouds associated with Gould's Belt. High dynamic range far …

Constraints on the distances to the dark clouds Chamaeleon I and II are investigated in
detail. A compilation of photometric data, spectral types and absolute magnitudes for field …

We present a new catalog of 406 dense cores optically selected by using the STScI Digitized
Sky Survey (DSS). In this catalog 306 cores have neither an embedded young stellar object …

Context. Chamaeleon is the southernmost low-mass star-forming complex within 200 pc
from the Sun. Its stellar population has been extensively studied in the past, but the current …

We present a survey of 28 molecular outflows driven by low-mass protostars, all of which are
sufficiently isolated spatially and/or kinematically to fully separate into individual outflows …

A new objective prism survey of the entire Chamaeleon I dark cloud and 2/3 of the
Chamaeleon II cloud has uncovered 26 new H-alpha emission line objects that were missed …

The goal of this paper is a detailed analysis of the dusty environment of Herbig Ae/Be stars
and FU Orionis objects. For this purpose we mapped 22 regions at 1.3 mm wavelength …