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More than half of all stars in the local Universe are found in massive spheroidal galaxies, which are characterized by old stellar populations with little or no current star formation. In present models, such galaxies appear rather late as…

Most stars, perhaps even all stars, form in crowded stellar environments. Such star forming regions typically dissolve within ten million years, while others remain bound as stellar groupings for hundreds of millions to billions of years,…

Earth and Planetary Astrophysics · Physics 2018-12-03 Francesco Flammini Dotti , Maxwell Xu Cai , Rainer Spurzem , M. B. N. Kouwenhoven

Extrasolar planets abound in almost any possible configuration. However, until five years ago, there was a lack of planets orbiting closer than 0.5 au to giant or subgiant stars. Since then, recent detections have started to populated this…

Earth and Planetary Astrophysics · Physics 2016-04-27 J. Lillo-Box , D. Barrado , A. C. M. Correia

The goal of searching back in cosmic time to find star formation during the epoch of reionization will soon be within reach. We assess the detectability of high-redshift galaxies by combining cosmological hydrodynamic simulations of galaxy…

The detection of lower mass planets now being reported via radial velocity and microlensing surveys suggests that they may be ubiquitous. If missions such as Kepler are able to confirm this, the detection and study of rocky planets via…

Earth and Planetary Astrophysics · Physics 2009-02-24 Philip M. Hinz , Scott Kenyon , Michael R. Meyer , Alan Boss , Roger Angel

Technological civilizations may rely upon large-scale photovoltaic arrays to harness energy from their host star. Photovoltaic materials, such as silicon, possess distinctive spectral features, including an "artificial edge" that is…

Earth and Planetary Astrophysics · Physics 2017-06-26 Manasvi Lingam , Abraham Loeb

Galaxies represent the visible fabric of the Universe and there has been considerable progress recently in both observational and theoretical studies. The underlying goal is to understand the present-day diversity of galaxy forms, masses…

Astrophysics · Physics 2007-05-23 Richard Ellis

With the example of Proxima Centauri we discuss the feasibility of detecting terrestrial planets (1 to a few M_Earth) using the high precision radial velocity (RV) technique. If a very high RV precision for M stars is achieved even planets…

The Era of the First Stars is one of the last unknown frontiers for exploration: a poorly understood billion years missing from our cosmological timeline. We have now developed several methods for finally filling in the lost billion years…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-02 Emma Chapman

One of the beneficial outcomes of searching for life in the Universe is that it grants greater awareness of our own problems here on Earth. Lack of contact with alien beings to date might actually comprise a null "signal" pointing humankind…

Popular Physics · Physics 2014-10-28 Eric J. Chaisson

The formation and evolution of galaxies is one of the great outstanding problems of astrophysics. Within the broad context of hierachical structure formation, we have only a crude picture of how galaxies like our own came into existence. A…

Astrophysics · Physics 2011-03-10 Ken Freeman , Joss Bland-Hawthorn

Exoplanets, short for `extra solar planets', are planets outside our solar system. They are objects with masses less than around 15 Jupiter-masses that orbit stars other than the Sun. They are small enough so they can not burn deuterium in…

Instrumentation and Methods for Astrophysics · Physics 2016-11-04 Muhammad Salman Khan , James Stewart Jenkins , Nestor Becerra Yoma

It is well-known that the chances of success of SETI depend on the longevity of technological civilizations or, more broadly, on the duration of the signs of their existence, or technosignatures. Here, we re-examine this general tenet in…

Instrumentation and Methods for Astrophysics · Physics 2021-04-28 Amedeo Balbi , Milan M. Ćirković

Using current observational data and simple dynamical modeling, we demonstrate that Omega Cen is not special among the Galactic globular clusters in its ability to produce and retain the heavy elements dispersed in the AGB phase of stellar…

The Fermi Paradox is the apparent contradiction between the high probability extraterrestrial civilizations' existence and the lack of contact with such civilizations. In general, solutions to Fermi's paradox come down to either estimation…

Popular Physics · Physics 2010-07-27 I. Bezsudnov , A. Snarskii

In about 40% of the Local Group galaxies star clusters have been detected so far, but the census is still incomplete. The properties of these clusters are briefly reviewed, and the impact of galaxy environment on the evolution and survival…

Astrophysics · Physics 2007-05-23 Eva K. Grebel

Our ability to explore the cosmos by direct contact has been limited to a small number of lunar and interplanetary missions. However, the NASA Starlight program points a path forward to send small, relativistic spacecraft far outside our…

In the search for life in the cosmos, transiting exoplanets are currently our best targets. In the search for life in the cosmos, transiting exoplanets are currently our best targets. With thousands already detected, our search is entering…

Earth and Planetary Astrophysics · Physics 2021-07-19 L. Kaltenegger , J. K. Faherty

Stellar populations, building blocks of galaxies, are direct tracers of the star formation history, the chemical enrichment and the assembly of galaxies in the Universe. They therfore allow us to understand how galaxies formed and evolved.…

Astrophysics · Physics 2007-07-30 A. Vazdekis , R. F. Peletier

This first part of Special Session 5 explored the current status of infrared-based observations of obscured and distant stellar clusters in the Milky Way galaxy. Recent infrared surveys, either serendipitously or using targeted searches,…

Solar and Stellar Astrophysics · Physics 2012-10-16 M. M. Hanson , D. Froebrich , F. Martins , A. -N. Chene , C. Rosslowe , A. Herrero , H. -J. Kim
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