Results 111 to 120 of about 3,076,442 (185)
Pre-main-sequence isochrones -- II. Revising star and planet formation timescales
We have derived ages for 13 young (
Bell, Cameron P. M. +4 more
core +1 more source
Accurate interpretation of observations relies on the interstellar dust extinction law, which also serves as a powerful diagnostic for probing dust properties.
Juan Deng +3 more
doaj +1 more source
ABSTRACT We present James Webb Space Telescope observations of M 4—the closest globular cluster—that probe the lower Main Sequence down to the hydrogen‐burning limit. The unveiled stellar sequence reaches much fainter luminosities than previously possible, revealing a few extremely red objects that are consistent with brown dwarfs as cool as Teff∼1000K$
L. R. Bedin +10 more
wiley +1 more source
Observations of young star clusters in a variety of galaxies have been used to constrain basic properties related to star formation, such as the fraction of stars found in clusters (Γ) and the shape of the cluster mass function (CMF).
Miranda Caputo +5 more
doaj +1 more source
Probing interstellar extinction near the 30 Doradus nebula with red giant stars
We have studied the interstellar extinction in a field of 3' x 3' located about 6' SW of 30 Doradus in the Large Magellanic Cloud (LMC). Hubble Space Telescope observations in the U, B, V, I and Halpha bands reveal patchy extinction in this field.
De Marchi, Guido +2 more
core +1 more source
Effective Temperatures of BA-Type Supergiants from SED Fitting
Supergiants are luminous post-main-sequence massive stars whose effective temperatures (Teff) are key inputs for stellar evolution and feedback studies.
Shakhida T. Nurmakhametova +7 more
doaj +1 more source
Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening
We present a simultaneous detection of gravitational magnification and dust reddening effects due to galactic halos and large-scale structure. The measurement is based on correlating the brightness of ~85,000 quasars at z>1 with the position of 20 ...
Abazajian +59 more
core +1 more source
To understand the nature of the NGC 146–King 14 cluster pair, we conducted a detailed photometric, astrometric, and dynamical study using multiwavelength data from Gaia DR3, Pan-STARRS1, WISE, and TESS.
D. Bisht +11 more
doaj +1 more source
Photometric distances to young stars in the inner Galactic disk. I. The L = 314$^{o}$ direction
The spiral structure of the Milky Way is nowadays receiving renewed attention thanks to the combined efforts of observational campaigns in different wavelength regimes, from the optical to the radio.
Ahumada +36 more
core +1 more source
We present BVi multiband high-cadence observations of a Type II supernova (SN) KSP-SN-2022c from a star-forming galaxy at z ≃ 0.041 from its infant to nebular phase. Early light-curve fitting with a single power law is consistent with the first detection
Nan Jiang +8 more
doaj +1 more source

