Exoplanets as sub-GeV dark matter detectors
We present exoplanets as new targets to discover dark matter (DM). Throughout the Milky
Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat …
Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat …
Modelling the Galactic interstellar extinction distribution in three dimensions
DJ Marshall, AC Robin, C Reylé, M Schultheis… - Astronomy & …, 2006 - aanda.org
Aims. The Two Micron All Sky Survey, along with the Stellar Population Synthesis Model of
the Galaxy, developed in Besançon, is used to calculate the extinction distribution along …
the Galaxy, developed in Besançon, is used to calculate the extinction distribution along …
Interstellar extinction law toward the galactic center III: J, H, KS bands in the 2MASS and the MKO systems, and 3.6, 4.5, 5.8, 8.0 μm in the Spitzer/IRAC system
S Nishiyama, M Tamura, H Hatano, D Kato… - The Astrophysical …, 2009 - iopscience.iop.org
We have determined interstellar extinction law toward the Galactic center (GC) at the
wavelength from 1.2 to 8.0 μm, using point sources detected in the IRSF/SIRIUS near …
wavelength from 1.2 to 8.0 μm, using point sources detected in the IRSF/SIRIUS near …
LIFTING THE DUSTY VEIL WITH NEAR-AND MID-INFRARED PHOTOMETRY. I. DESCRIPTION AND APPLICATIONS OF THE RAYLEIGH–JEANS COLOR EXCESS …
SR Majewski, G Zasowski… - The Astrophysical …, 2011 - iopscience.iop.org
ABSTRACT The Milky Way (MW) remains a primary laboratory for understanding the
structure and evolution of spiral galaxies, but typically we are denied clear views of MW …
structure and evolution of spiral galaxies, but typically we are denied clear views of MW …
Discrete sources as the origin of the Galactic X-ray ridge emission
M Revnivtsev, S Sazonov, E Churazov, W Forman… - Nature, 2009 - nature.com
An unresolved X-ray glow (at energies above a few kiloelectronvolts) was discovered about
25 years ago and found to be coincident with the Galactic disk—the Galactic ridge X-ray …
25 years ago and found to be coincident with the Galactic disk—the Galactic ridge X-ray …
The effective temperature scale of FGK stars. I. Determination of temperatures and angular diameters with the infrared flux method
I Ramírez, J Meléndez - The Astrophysical Journal, 2005 - iopscience.iop.org
The infrared flux method (IRFM) has been applied to a sample of 135 dwarf and 36 giant
stars covering the following regions of the atmospheric parameter space:(1) the metal-rich …
stars covering the following regions of the atmospheric parameter space:(1) the metal-rich …
The interstellar extinction law toward the Galactic center. II. V, J, H, and Ks bands
S Nishiyama, T Nagata, M Tamura… - The Astrophysical …, 2008 - iopscience.iop.org
We have determined the ratios of total to selective extinction directly from observations in the
optical V band and near-infrared J band toward the Galactic center. The OGLE (Optical …
optical V band and near-infrared J band toward the Galactic center. The OGLE (Optical …
Interstellar extinction
GA Gontcharov - Astrophysics, 2016 - Springer
This review describes our current understanding of interstellar extinction. This differ
substantially from the ideas of the 20th century. With infrared surveys of hundreds of millions …
substantially from the ideas of the 20th century. With infrared surveys of hundreds of millions …
Reddening and metallicity maps of the Milky Way bulge from VVV and 2MASS-I. The method and minor axis maps
OA Gonzalez, M Rejkuba, M Zoccali, E Valenti… - Astronomy & …, 2011 - aanda.org
Context. The Milky Way bulge is the nearest galactic bulge and the best laboratory for
studies of stellar populations in spheroids based on individual stellar abundances and …
studies of stellar populations in spheroids based on individual stellar abundances and …
Tracing the Galactic anticenter stellar stream with 2MASS M giants
HJ Rocha-Pinto, SR Majewski… - The Astrophysical …, 2003 - iopscience.iop.org
The recently discovered, ringlike structure just outside the Galactic disk in Monoceros is
detected and traced among 2MASS M giant stars. We have developed a method to recover …
detected and traced among 2MASS M giant stars. We have developed a method to recover …