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 …
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 …
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 …
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 …
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 …
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 …
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 …
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 …
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 …