The dust attenuation law in galaxies
S Salim, D Narayanan - Annual Review of Astronomy and …, 2020 - annualreviews.org
Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …
mechanisms that shape them are among the fundamental questions of extragalactic …
The cosmological constant and dark energy
PJE Peebles, B Ratra - Reviews of modern physics, 2003 - APS
Physics welcomes the idea that space contains energy whose gravitational effect
approximates that of Einstein's cosmological constant, Λ; today the concept is termed dark …
approximates that of Einstein's cosmological constant, Λ; today the concept is termed dark …
The ATLAS3D project – XV. Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and …
We study the volume-limited and nearly mass-selected (stellar mass M stars≳ 6× 109 M⊙)
ATLAS3D sample of 260 early-type galaxies (ETGs, ellipticals Es and lenticulars S0s). We …
ATLAS3D sample of 260 early-type galaxies (ETGs, ellipticals Es and lenticulars S0s). We …
Maps of dust infrared emission for use in estimation of reddening and cosmic microwave background radiation foregrounds
DJ Schlegel, DP Finkbeiner, M Davis - The Astrophysical Journal, 1998 - iopscience.iop.org
We present a full-sky 100 μ m map that is a reprocessed composite of the COBE/DIRBE and
IRAS/ISSA maps, with the zodiacal foreground and confirmed point sources removed …
IRAS/ISSA maps, with the zodiacal foreground and confirmed point sources removed …
A relationship between nuclear black hole mass and galaxy velocity dispersion
K Gebhardt, R Bender, G Bower… - The Astrophysical …, 2000 - iopscience.iop.org
We describe a correlation between the mass M bh of a galaxy's central black hole and the
luminosity-weighted line-of-sight velocity dispersion σ e within the half-light radius. The …
luminosity-weighted line-of-sight velocity dispersion σ e within the half-light radius. The …
The growth of massive galaxies since z= 2
PG Van Dokkum, KE Whitaker, G Brammer… - The Astrophysical …, 2010 - iopscience.iop.org
We study the growth of massive galaxies from z= 2 to the present using data from the
NOAO/Yale NEWFIRM Medium Band Survey. The sample is selected at a constant number …
NOAO/Yale NEWFIRM Medium Band Survey. The sample is selected at a constant number …
Supermassive black holes in galactic nuclei: past, present and future research
L Ferrarese, H Ford - Space Science Reviews, 2005 - Springer
This review discusses the current status of supermassive black hole research, as seen from
a purely observational standpoint. Since the early '90s, rapid technological advances, most …
a purely observational standpoint. Since the early '90s, rapid technological advances, most …
The SBF survey of galaxy distances. IV. SBF magnitudes, colors, and distances
JL Tonry, A Dressler, JP Blakeslee… - The Astrophysical …, 2001 - iopscience.iop.org
We report data for I-band surface brightness fluctuation (SBF) magnitudes,(VI) colors, and
distance moduli for 300 galaxies. The survey contains E, S0, and early-type spiral galaxies …
distance moduli for 300 galaxies. The survey contains E, S0, and early-type spiral galaxies …
The centers of early-type galaxies with HST. IV. Central parameter relations
We analyze Hubble Space Telescope surface-brightness profiles of 61 elliptical galaxies
and spiral bulges (hot galaxies). Luminous hot galaxies have cuspy cores with steep outer …
and spiral bulges (hot galaxies). Luminous hot galaxies have cuspy cores with steep outer …
Old stellar populations. VI. absorption-line spectra of galaxy nuclei and globular clusters
We present absorption-line strengths on the Lick/IDS line-strength system of 381 galaxies
and 38 globular clusters in the 4000–6400 Å region. All galaxies were observed at Lick …
and 38 globular clusters in the 4000–6400 Å region. All galaxies were observed at Lick …