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The XMM-Newton Bright Serendipitous Survey
The XMM-Newton Bright Serendipitous Survey

... In the last years the XMM-Newton images have been reprocessed with improved versions of the SAS and the astrometry has been refined and corrected. We have thus recomputed the X-ray-optical offsets using the improved X-ray positions included in the preliminary version of the second XMM-Newton Serendi ...
Report from the Subaru Telescope for External
Report from the Subaru Telescope for External

... galaxy and primeval clusters of galaxies, the lowest mass exoplanet GJ 504 b, proto-planetary disks with various morphologies. In addition, frontier pieces of research ...
THE OFFSET AND HOST LIGHT DISTRIBUTIONS OF LONG
THE OFFSET AND HOST LIGHT DISTRIBUTIONS OF LONG

... In addition to the tension between the results of previous studies, and the relatively small samples used in these studies, it is important to note other potential challenges. First, the aforementioned studies were based on LGRB samples collected from multiple satellites using different trigger crit ...
Mid-infrared Properties of Seyfert Galaxies: the IRAS 12um Sample
Mid-infrared Properties of Seyfert Galaxies: the IRAS 12um Sample

... Using the infrared to study this issue offers a number of advantages the more important of which is… SHAO - Oct 2010 ...
OBSERVATIONS OF PHYSICAL PROCESSES IN
OBSERVATIONS OF PHYSICAL PROCESSES IN

... to get me to this point in my life. Thanks to my brothers for continuing to be their annoying selves. Thanks to Emi for making it work from so far away and letting me be a house husband while I search for a job. Thanks to a former stranger who let me borrow her tent. Thanks to Raft, Toad, and the SH ...
WFC3 Science White Paper - Space Telescope Science Institute
WFC3 Science White Paper - Space Telescope Science Institute

... A primary legacy of the Hubble Space Telescope (HST), both scientifically and in the public eye, will be the spectacular images it produces of the astronomical sky. Its cameras have been among the most productive instruments in the history of astronomy. As HST begins a second decade of operations, i ...
Galaxy Disks Further
Galaxy Disks Further

... The significance of internal secular evolution for the evolution of disks has become clear in recent years. The presence of oval distortions, bars, and spiral structure can have a profound effect on the changing structure of disks, as has been extensively reviewed by Kormendy & Kennicutt (2004) and ...
- Isaac Newton Group of Telescopes
- Isaac Newton Group of Telescopes

... was confirmed to coincide with that of the stars of the cluster and, later, a precise photometric characterization was achieved. Several high resolution spectra between 600 and 900 nm were obtained with the WHT. These spectra confirmed the discovery of one of the coldest quasi-stellar objects known ...
Abstract The Star Formation History of Low Surface Brightness Galaxies
Abstract The Star Formation History of Low Surface Brightness Galaxies

... The star formation histories of low surface brightness galaxies are interesting but poorly constrained. These objects tend to be rather blue, contradicting the initial impression that they may simply be faded remnants of higher surface brightness galaxies whose star formation has finished. Other sce ...
Annual Report 2011 - Max Planck Institute for Astrophysics
Annual Report 2011 - Max Planck Institute for Astrophysics

... Planck Surveyor is a medium-sized ESA satellite mission to map the Cosmic Microwave Background. It was launched in May 2009 and has been operating nominally on station at L2 since late August 2009. ’First light’ was in September 2009. Already in July 2010 the international consortium released the fi ...
IRAM Annual Report 2014
IRAM Annual Report 2014

... companions, even in a relatively poor cluster such as the one associated with IRAS 20126+4104. This might explain why disks around O-stars, surrounded by rich clusters, have been until now so elusive. It is to expect that in the long term NOEMA’s high sensitivity and broader range of capabilities wi ...
Revising the census of low luminosity AGN
Revising the census of low luminosity AGN

... A LOW EW (~1 Å) IS CHARACTERISTIC OF STELLAR PROCESSES AGN 10 - Roma 10/09/2012 ...
probing quasar environments with tunable filter
probing quasar environments with tunable filter

... MRC B1256-243 lack the sensitivity to probe deep into the quasar environment, but detect a number of extremely luminous objects. In BR B0019-1522, we show convincing evidence of a protocluster, including both galaxy and star formation rate densities an order of magnitude higher than that observed in ...
GRB prompt emission
GRB prompt emission

... Using GRBs as Cosmological Probes Gamma-Ray Bursts are observed at extremely high redshifts and can be used to study the early universe. • Star Formation History • Beacons to direct large telescopes to study nascent galaxies • Studies of intervening material between us and GRB – akin to quasar abso ...
GRB prompt emission
GRB prompt emission

... Using GRBs as Cosmological Probes Gamma-Ray Bursts are observed at extremely high redshifts and can be used to study the early universe. • Star Formation History • Beacons to direct large telescopes to study nascent galaxies • Studies of intervening material between us and GRB – akin to quasar abso ...
Stars, Galaxies, Superuniverses and the Urantia Book, by Frederick
Stars, Galaxies, Superuniverses and the Urantia Book, by Frederick

... "Your world, Urantia, is one of many similar inhabited planets which comprise the local universe of Nebadon. This universe, together with similar creations, makes up the superuniverse of Orvonton, from whose capital, Uversa, our commission hails. Orvonton is one of the seven evolutionary superuniver ...
Observational Studies of Interacting Galaxies and the Development
Observational Studies of Interacting Galaxies and the Development

... Interacting galaxies are thought to be the essential building blocks of elliptical galaxies under the hierarchical galaxy formation scenario. The goal of my dissertation is to broaden our understanding of galaxy merger evolution through both observational studies and instrument developments. Observa ...
Annual Report 2006/2007
Annual Report 2006/2007

... halos of unknown constitution. Astronomers are able to look back in time, by observing galaxies at ever greater distances. Because light travels at finite velocity, distant objects are seen at a time when the Universe was young. The expansion of the Universe causes light to be redshifted, so that th ...
Star Formation in the Milky Way and Nearby Galaxies Further
Star Formation in the Milky Way and Nearby Galaxies Further

... list of key questions in the field. Some have been or will be addressed by other reviews. Some are best answered by observations of other galaxies; some can be addressed only by observations of local star-forming regions in the MW. For each question, we list sections in this review where we review t ...
IRAM Annual Report 2011
IRAM Annual Report 2011

... and redshift (z=5.2429). The dominant lens is a foreground z=0.63 galaxy, not the cluster itself. The source has a far-infrared (FIR) luminosity of LFIR= 1.1 1014μ L⊙, where μ~11 is the magnification factor. Combes reported the redshift identification through CO lines with the IRAM 30m telescope, an ...
Rich
Rich

... vary from galaxy to galaxy. • Opportunity: Galex grism mode in Far-UV (FUV) used to discover the first known sample of low redshift LAE galaxies. Instead of studying LAEs at z~4, study them at z~0.3 • Goal: Analyze photometry and spectroscopy of a local z~0.3 sample of ~76 LAEs and 107 non-LAEs to : ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... regimes capture dust emission because of the relatively low grain temperature, 20-60 K. Such emission is important within our Solar System, in proto-planetary disks where we believe planetary systems like our own are forming, and throughout the disk of the Mil ...
Teaching Tips Table of Contents - Hubble Deep Field
Teaching Tips Table of Contents - Hubble Deep Field

... Educators should allow approximately 45-55 minutes for the Orientation section of the activity and approximately 45-55 minutes for each of the activity’s four “Academy” levels. About 30-40 minutes should be allotted for students to complete the readings in the Deeper Views section. Depending on the ...
The old globular cluster system of the dIrr galaxy NGC 1427A in the
The old globular cluster system of the dIrr galaxy NGC 1427A in the

... In all these models, the GCSs of low-mass dwarf galaxies, the most numerous galaxy type in galaxy clusters (Sandage 2005, and references therein), are envisioned as the building blocks of the GCSs of the more massive galaxies. At present the role of the GCSs of dIrr galaxies in the frame of galaxy f ...
FLARE SWG theme 3: high
FLARE SWG theme 3: high

... Large-scale clustering analyses with respect to galaxies – bias and constraints on BH seed formation? Mpc-scale environment around first quasars using FLARE IFU: co-eval galaxy and other z>6 quasar/AGN connections (multiple growing BHs)? Evidence for quasar outflows (e.g., broad CIV absorption troug ...
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Pea galaxy



A Pea galaxy, also referred to as a Pea or Green Pea, might be a type of Luminous Blue Compact Galaxy which is undergoing very high rates of star formation. Pea galaxies are so-named because of their small size and greenish appearance in the images taken by the Sloan Digital Sky Survey (SDSS).Pea Galaxies were first discovered in 2007 by the volunteer users within the forum section of the online astronomy project Galaxy Zoo (GZ).
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