The survey is led by Doug Johnstone, Research Officer at the National Research Council of Canada and Greg Herczeg, Professor at Peking University (China), and is supported by an international
team of astronomers from Canada, China, Korea, Japan, Taiwan and the United Kingdom.
A team of astronomers from the University of Cambridge have identified nine new dwarf satellites orbiting the Milky Way, the largest number ever discovered at once.
Last month an amateur
team of astronomers from the La Sagra Sky Survey Observatory in southeast Spain discovered an asteroid roughly 150 feet wide as it -LSB-...]
Discovery of the system's extraordinary properties was made by
a team of astronomers from Vanderbilt and Harvard with the assistance of colleagues at Lehigh, Ohio State and Pennsylvania State universities, Las Cumbres Observatory Global Telescope Network and the American Association of Variable Star Observers and is described in a paper accepted for publication in the Astronomical Journal.
A team of astronomers from Germany and Britain have discovered a new planet, which has the potential to be habitable.
A team of astronomers from the U.S. and Canada, including four professors from the University [continue reading]
Measurements taken by
a team of astronomers from the Universities of Geneva and Bern are given in the framework of the PlanetS NCCR; the figures come from observations made over sodium spectral lines.
Using the National Science Foundation's Very Long Baseline Array (VLBA) of radio telescopes, an international
team of astronomers from the United States and Taiwan studied the area generally thought to mark the Galactic center.
Now, a new study by
a team of astronomers from France, Israel and Hawaii demonstrates a novel approach.
The measurements confirm observations by
another team of astronomers from the Netherlands, which detected the polarized bursts using the William E. Gordon Telescope at the Arecibo Observatory in Puerto Rico.
Three new planets classified as habitable - zone super-Earths are amongst eight new planets discovered orbiting nearby red dwarf stars by an international
team of astronomers from the UK and Chile.
A team of astronomers from the National Astronomical Observatory of Japan (NAOJ) and SOKENDAI (Graduate University of Advanced Studies, Japan) are tracking velocity structures and gaseous metallicities in galaxies in two protoclusters located in the direction of the constellation Serpens.
Not exact matches
In two studies, international
teams of astronomers suggest that recent images
from NASA's Chandra X-ray Observatory
of two pulsars — Geminga and B0355 +54 — may help shine a light on the distinctive emission signatures
of pulsars, as well as their often perplexing geometry.
An international
team of astronomers has determined that Centaurus A, a massive elliptical galaxy 13 million light - years
from Earth, is accompanied by a number
of dwarf satellite galaxies orbiting the main body in a narrow disk.
Now, a
team of astronomers has used position and velocity data
from the Sloan Digital Sky Survey as well as computer simulations
of stellar evolution in the Large Magellanic Cloud (LMC, pictured above), a small satellite galaxy near the Milky Way, to show that these speeding stars may come
from there.
So one
team of astronomers used data
from the Gaia space observatory to simulate the interiors
of solar - type stars, which are similar in mass and age to our own sun.
A
team of European
astronomers says the secret to their cohesion is a cushion
of dark matter that protects them
from the gravitational tug -
of - war outside.
In fact, Swift X-ray and optical observations were carried out two days after FRB 131104, thanks to prompt analysis by radio
astronomers (who were not aware
of the gamma - ray counterpart) and a nimble response
from the Swift mission operations
team, headquartered at Penn State.
In 2012 and 2014 a
team led by an
astronomer from Paris Observatory took a second look at the auroras using the ultraviolet capabilities
of the Space Telescope Imaging Spectrograph (STIS) installed on Hubble.
To solve this problem,
astronomers from Daniel Schaerer's research group at the Department
of Astronomy
of the Faculty
of Sciences, and an international
team proposed to observe «green pea» galaxies.
A
team led by
astronomer Kenji Hamaguchi
of NASA's Goddard Space Flight Center in Greenbelt, Maryland, used the XMM - Newton and Chandra x-ray satellites to study a stellar nursery just 550 light - years
from Earth.
In the following years, the
team that included Dr. Marilyn Latour, an
astronomer from the Dr. Remeis - Sternwarte Bamberg, the astronomical institute
of Friedrich - Alexander - Universität Erlangen - Nürnberg (FAU), studied these stars in more detail and concluded that they had stumbled upon a new class
of variable star.
An international
team of astronomers including researchers
from the University
of British Columbia has discovered a new dwarf planet orbiting in the disk
of small icy worlds beyond Neptune.
The
team calculates an age
of only 400 - 600 million years old, which agrees with the age estimated
from its rotation period (a technique pioneered by CfA
astronomer Soren Meibom).
A
team of British and American
astronomers used data
from several telescopes on the ground and in space — among them the NASA / ESA Hubble Space Telescope — to study the atmosphere
of the hot, bloated, Saturn - mass exoplanet WASP - 39b, about 700 light - years
from Earth.
Following up on the discovery, an international
team of scientists led by the Swiss
astronomer Vincent Bourrier
from the Observatoire de l'Université de Genève, used the Space Telescope Imaging Spectrograph (STIS) on the NASA / ESA Hubble Space Telescope to study the amount
of ultraviolet radiation received by the individual planets
of the system.
Other papers in the package also touch on the presence
of water ice on Ceres, which had already been reported by the Dawn
team and by
astronomers observing the dwarf planet
from afar.
Using archival data
from the Sloan Digital Sky Survey, and the XMM - Newton and Chandra X-ray telescopes, a
team of astronomers have discovered a gigantic black hole, which is probably destroying and devouring a big star in its vicinity.
The key observation
from the new research is that the small dip in the HAT - P - 7 b light curve when the planet passes behind its star «is roughly equivalent to the signal
of an Earth - size planet when it passes in front
of its parent star,» says Paul Kalas, an
astronomer at the University
of California, Berkeley, who is not part
of the Kepler
team.
The new COS observations build and expand on the findings
of a 2015 Hubble study by the same
team, in which
astronomers analyzed the light
from one quasar that pierced the base
of the bubble.
«Each family member drifts away
from the center
of the family in a way that depends on its size, with small guys drifting faster and further than the larger guys,» said
team leader Marco Delbo, an
astronomer from the Observatory
of Cote d'Azur in Nice, France.
A
team of astronomers has combined new observations
of Gliese 667C with existing data
from HARPS at ESO's 3.6 - metre telescope in Chile, to reveal a system with at least six planets.
A
team of astronomers led by John Webb
of the University
of New South Wales has been measuring how the light
from quasars is absorbed by gas clouds that lie between them and us but are still billions
of light - years away, and thus did their absorbing billions
of years ago.
Using data captured by ALMA in Chile and
from the ROSINA instrument on ESA's Rosetta mission, a
team of astronomers has found faint traces
of the chemical compound [Freon - 40]--(CH3Cl), also known as methyl chloride and chloromethane, around both the infant star system IRAS 16293 - 2422, about 400 light - years away, and the famous comet 67P / Churyumov - Gerasimenko (67P / C - G) in our own Solar System.
But a
team of astronomers recently discovered something odd enough to make even their most jaded colleagues take notice: a vast fountain
of antimatter that appears to be spewing
from our galaxy's center.
The first earthly pieces
of Vesta were identified only in 1970, when a
team of astronomers studying light reflected
from the asteroid's surface found that its spectrum — which reveals the minerals present — perfectly matched that
of a certain distinct class
of meteorite.
An interdisciplinary
team of UvA physicists and
astronomers proposed to search for primordial black holes in our galaxy by studying the X-ray and radio emission that these objects would produce as they wander through the galaxy and accrete gas
from the interstellar medium.
To spot the black hole's event horizon, a
team of astronomers — led by Michael Garcia and Ramesh Narayan
of the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts — watched what happened as a black hole stole gas away
from a nearby star.
So using the Hubble Space Telescope, MIT
astronomer Julien de Wit and his colleagues, including some members
from Grimm's
team, observed the four middle planets as they passed in front
of the star.
A possible answer comes
from a new model
of the black hole's feeding behavior, presented by a
team led by Roman Shcherbakov, an x-ray
astronomer at Harvard University.
Lawrence Rudnick, the
astronomer who led the
team that found the void, was studying data
from the Very Large Array, a network
of 27 radio antennas in New Mexico, when he spotted a gap in the constellation Eridanus where radio signals
from galaxies appear unusually faint.
Last February a
team of astronomers reported detecting an afterglow
from a mysterious event called a fast radio burst, which would pinpoint the precise position
of the burst's origin, a longstanding goal in studies
of these mysterious events.
Upon closer examination
of the data — compiled
from nearly 500 hours
of observation by the 64 - meter Parkes radio telescope in Australia — a
team led by
astronomer Duncan Lorimer
of West Virginia University in Morgantown estimated that the blast actually came
from about 3 billion light - years away.
An international
team of astronomers, led by Imperial College London, used a new way
of combining data
from the two European Space Agency satellites, Planck and Herschel, to identify more distant galaxy clusters than has previously been possible.
The Magellanic Clouds, the two largest satellite galaxies
of the Milky Way, appear to be connected by a bridge stretching across 43,000 light years, according to an international
team of astronomers led by researchers
from the University
of Cambridge.
Now, a
team of astronomers says they have found another one, not quite as big, orbiting 200 light - years
from the center
of the Milky Way.
And when matter ejected
from the second explosion caught up with the debris
from the first, the resulting collision produced an extremely bright flash, which is what
astronomers observed with SN 2006gy, the
team reports in the 15 November issue
of Nature.
Hendrik Hildebrandt
from the Argelander - Institut für Astronomie in Bonn, Germany and Massimo Viola
from the Leiden Observatory in the Netherlands led a
team of astronomers [1]
from institutions around the world who processed images
from the Kilo Degree Survey (KiDS), which was made with ESO's VLT Survey Telescope (VST) in Chile.
«Last Sunday, after seven years in space traveling nearly three billion miles, Stardust landed in the Great Salt Lake Desert with a treasure
from when the solar system formed 4.6 billion years ago,» says
astronomer Donald Brownlee
of the University
of Washington, who led the Stardust
team.
The finding, by an international
team of astronomers, including Professor Geraint Lewis
from the University
of Sydney's School
of Physics, is announced today in Nature.