The aim of this paper is to quantitatively testify the 'small-scale sequential star
formation'hypothesis in and around bright-rimmed clouds (BRCs). As a continuation of the …

The aim of this paper is to present the results of photometric investigations of the central
cluster of the W5 EH ii region as well as a follow-up study of the triggered star formation in …

We present results on the star formation activity of an optically obscured region containing
an embedded cluster (S255-IR) and molecular gas between two evolved H ii regions, S255 …

We present UBVI c CCD photometry of the young open cluster Stock 8 with the aim of
studying its basic properties such as the amount of interstellar extinction, distance, age …

Context. Star-forming complexes are large structures exhibiting massive star-formation at
different stages of evolution, from dense cores to well-developed H ii regions. They are very …

We present optical photometric and polarimetric observations of stars toward NGC 1931 with
the aim of deriving cluster parameters such as distance, reddening, age, and …

Deep and wide-field optical photometric observations along with multiwavelength archival
data sets have been employed to study the physical properties of the cluster NGC 6910. The …

Infrared dark clouds are ideal laboratories for studying the initial processes of high-mass star
and star-cluster formation. We investigated the star formation activity of an unexplored …

We report the observational findings of the Sh2-112 H ii region by using the multiwavelength
data analysis ranging from optical to radio wavelengths. This region is powered by the …

Abstract The Planck Galactic Cold Clumps (PGCCs) are possible representations of the
initial conditions and very early stages of star formation. With the objective of understanding …