The initial mass function of the massive star-forming region NGC 3603 from near-infrared adaptive optics observations

Y Harayama, F Eisenhauer… - The Astrophysical Journal, 2008 - iopscience.iop.org
We study the initial mass function (IMF) of one of the most massive Galactic star-forming
regions NGC 3603 to answer a fundamental question in current astrophysics: is the IMF …

Testing the role of environmental effects on the initial mass function of low-mass stars

B Damian, J Jose, MR Samal, E Moraux… - Monthly Notices of …, 2021 - academic.oup.com
In the star-formation process, the vital impact of environmental factors such as feedback from
massive stars and stellar density on the form of the initial mass function (IMF) at the low …

Initial mass function variability from the integrated light of diverse stellar systems

CM Cheng, A Villaume, ML Balogh… - Monthly Notices of …, 2023 - academic.oup.com
We present a uniform analysis of the stellar initial mass function (IMF) from integrated light
spectroscopy of 15 compact stellar systems (11 globular clusters in M31 and 4 ultra compact …

The Villafranca catalog of Galactic OB groups-I. Systems with O2–O3. 5 stars

JM Apellániz, PC Bellido, RH Barbá, RF Aranda… - Astronomy & …, 2020 - aanda.org
Context. The spectral classifications of the Galactic O-Star Spectroscopic Survey (GOSSS)
and the astrometric and photometric data from Gaia have significantly improved our ability to …

The secrets of the nearest starburst cluster. II. The present-day mass function in NGC 3603

A Stolte, W Brandner, B Brandl… - The Astronomical …, 2006 - iopscience.iop.org
Abstract Based on deep Very Large Telescope Infrared Spectrometer and Array Camera
JHK photometry, we have derived the present-day mass function (MF) of the central starburst …

The initial mass function and stellar content of NGC 3603

H Sung, MS Bessell - The Astronomical Journal, 2004 - iopscience.iop.org
We present UBVRI and H α photometry of the extremely compact, starburst cluster NGC
3603. Ground-based images, Hubble Space Telescope (HST) archival data, as well as …

The chemical abundance of the very metal-rich old open clusters NGC 6253 and NGC 6791

E Carretta, A Bragaglia, RG Gratton - Astronomy & Astrophysics, 2007 - aanda.org
Aims. In the framework of a project aiming at homogeneously deriving the properties (age,
distance, reddening, and detailed chemical abundances) of a large sample of old open …

The spectrum of the very massive binary system WR 20a (WN6ha+ WN6ha): Fundamental parameters and wind interactions

G Rauw, PA Crowther, M De Becker, E Gosset… - Astronomy & …, 2005 - aanda.org
We analyse the optical spectrum of the very massive binary system WR 20a (WN6ha+
WN6ha). The most prominent emission lines, Hα and He ii λ 4686, display strong phase …

The Massive Star Content of NGC 3603

NW Melena, P Massey, NI Morrell… - The Astronomical …, 2008 - iopscience.iop.org
We investigate the massive star content of NGC 3603, the closest known giant H ii region.
We have obtained spectra of 26 stars in the central cluster using the Baade 6.5 m telescope …

Uncertainties of synthetic integrated colors as age indicators

KY Sukyoung - The Astrophysical Journal, 2003 - iopscience.iop.org
We investigate the uncertainties in the synthetic integrated colors of simple stellar
populations, currently the most popular method of estimating the ages of unresolved stellar …