Annual Review of Astronomy and Astrophysics

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Interstellar Polycyclic Aromatic Hydrocarbon Molecules
Annual Review of Astronomy and Astrophysics - Tập 46 Số 1 - Trang 289-337 - 2008
A. G. G. M. Tielens
Large polycyclic aromatic hydrocarbon (PAH) molecules carry the infrared (IR) emission features that dominate the spectra of most galactic and extragalactic sources. This review surveys the observed mid-IR characteristics of these emission features and summarizes laboratory and theoretical studies of the spectral characteristics of PAHs and the derived intrinsic properties of emitting interstellar... hiện toàn bộ
High-Mass Star and Massive Cluster Formation in the Milky Way
Annual Review of Astronomy and Astrophysics - Tập 56 Số 1 - Trang 41-82 - 2018
F. Motte, Sylvain Bontemps, F. Louvet
This review examines the state-of-the-art knowledge of high-mass star and massive cluster formation, gained from ambitious observational surveys, which acknowledges the multiscale characteristics of these processes. After a brief overview of theoretical models and main open issues, we present observational searches for the evolutionary phases of high-mass star formation, first among high-luminosit... hiện toàn bộ
Cosmology with the Sunyaev-Zel’dovich Effect
Annual Review of Astronomy and Astrophysics - Tập 40 Số 1 - Trang 643-680 - 2002
J. E. Carlstrom, G. P. Holder, Erik D. Reese
▪ Abstract  The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-scale structure of the universe as traced by massive clusters of galaxies. As a spectral distortion of the cosmic microwave background, the SZE is insensitive to the redshift of the galaxy cluster, making it well-suited for studies of clusters at all redshifts, and especially at reasonably high redshifts (z > 1)... hiện toàn bộ
Asymptotic Giant Branch Evolution and Beyond
Annual Review of Astronomy and Astrophysics - Tập 21 Số 1 - Trang 271-342 - 1983
Icko Iben, A. Renzini
The Evolution and Structure of Pulsar Wind Nebulae
Annual Review of Astronomy and Astrophysics - Tập 44 Số 1 - Trang 17-47 - 2006
B. M. Gaensler, Patrick Slane
Pulsars steadily dissipate their rotational energy via relativistic winds. Confinement of these outflows generates luminous pulsar wind nebulae, seen across the electromagnetic spectrum in synchrotron and inverse Compton emission and in optical emission lines when they shock the surrounding medium. These sources act as important probes of relativistic shocks, particle acceleration, and interstella... hiện toàn bộ
The Cosmological Constant
Annual Review of Astronomy and Astrophysics - Tập 30 Số 1 - Trang 499-542 - 1992
Sean M. Carroll, A. G. W. Cameron, Edwin L. Turner
Microlensing Surveys for Exoplanets
Annual Review of Astronomy and Astrophysics - Tập 50 Số 1 - Trang 411-453 - 2012
B. Scott Gaudi
Unlike most other planet-detection techniques, gravitational microlensing does not rely on detection of photons from either the host or the planet. Rather, planets are discovered by their gravitational perturbation of light from a more distant source. I review the fundamental concepts of microlensing planet searches and discuss their practical application. I show how the strengths and peculiaritie... hiện toàn bộ
Sources of Relativistic Jets in the Galaxy
Annual Review of Astronomy and Astrophysics - Tập 37 Số 1 - Trang 409-443 - 1999
I. F. Mirabel, L. F. Rodríguez
▪ Abstract  Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact sources are found by means of multiwavelength observations with ground-based telescopes. The X-ray emission probes the inner accretion disk and immediate surroundings of the compact object, whereas the sy... hiện toàn bộ
Thermonuclear Reaction Rates
Annual Review of Astronomy and Astrophysics - Tập 5 Số 1 - Trang 525-570 - 1967
William A. Fowler, Georgeanne R. Caughlan, Barbara A. Zimmerman
The Chemical Composition of the Sun
Annual Review of Astronomy and Astrophysics - Tập 47 Số 1 - Trang 481-522 - 2009
M. Asplund, N. Grevesse, A. J. Sauval, Pat Scott
The solar chemical composition is an important ingredient in our understanding of the formation, structure, and evolution of both the Sun and our Solar System. Furthermore, it is an essential reference standard against which the elemental contents of other astronomical objects are compared. In this review, we evaluate the current understanding of the solar photospheric composition. In particular, ... hiện toàn bộ
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