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Nova Vul05
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Magnitude 15.8 Variable Vul 05 a new variable near M27 in the constellation Vulpecula, was discovered by Joerg Hanisch and Hans-Goeran Lindberg on August 21, 2005.
Position(2000): R.A. = 19h 59m 51.29s D...
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NGC 7129
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The stellar nursery NGC 7129 lies 3,000 light-years away in the constellation Cepheus[img]http://antwrp.gsfc.nasa.gov/apod/image/0508/...
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47 Ursa Major
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Could the 47 UMa Planetary System be a Second Solar System: predicting the Earth-like planets.
Authors:[img]http://photos22.flickr.com/32922654_d822f02...
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HD143436
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A dim yellow star in the constellation Serpens Caput may be nearly identical to the Sun, say astronomers in South Carolina and Hawaii. The star could therefore host a life-bearing planet like Earth.
In 1997, astronomers in Brazil identified a solar twin in Scorpius named 18 Scorpii[/...
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NOVA SCORPII 2005
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1737-34 NOVA SCORPII 2005
A Nova in Scorpius was discovered yesterday, July 25, at magnitude 9.
The nova was discovered Independently by the ASAS-3 survey (Grzegorz Pojmanski, Warsaw University Astronomical Observatory) and Hideo Nishimura, Kakegawa, Shizuoka-ken, Japan.
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SDSS J090745.0+024507
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Title: The Hypervelocity Star SDSS J090745.0+024507 is a Short-Period Variable
Authors: Cesar I. Fuentes, K. Z. Stanek, B. Scott Gaudi, Brian A. McLeod,
Slavko B. Bogdanov, Joel D. Hartman, Ryan C. Hickox, Matthew J. Holman
Researchers have taken high-precision photo...
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LAB-2 Superwinds
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A team of astronomers, led by the University of Durham, has discovered the aftermath of a spectacular explosion in a galaxy 11.5 billion light years away.
Their observations, reported today (14th July 2005) in the journal Nature provide the most direct evidence yet of a galaxy being al...
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OGLE-TR-10
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High-precision Transit Photometry of OGLE-TR-10
Authors: Matthew J. Holman, Joshua N. Winn, K.Z. Stanek, Guillermo Torres, Dimitar D. Sasselov, R. Lynne Allen, Wesley Fraser
Researchers present B and I photometry of OGLE-TR-10 during transits of its gi...
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Young, Jupiter-Mass Objects
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Young, Jupiter-Mass Objects in Ophiuchus
Authors: K. N. Allers, D. T. Jaffe, N. S. van der Bliek, F. Allard, I. Baraffe
It appeared in the proceedings of "The Spitzer Space Telescope: New Views of the Cosmos" (9-12 November 2004)
By using 3.5 to 8 micron data from the [b...
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Infrared Coronagraphic Survey
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An Infrared Coronagraphic Survey for Substellar Companions
Authors: P.Lowrance (SSC), E. E. Becklin (UCLA), G. Schneider (UofA), D. Kirkpatrick (IPAC), A.Weinberger (Carnegie), B. Zuckerman (UCLA), C.Dumas (ESO), J.L.Beuzit (Grenoble), P.Plait (Sonoma State), E.Malumuth (Go...
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Nova AQL 05
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Nova AQL 05
A possible nova has been reported in Aquila.
The nova has an amplitude grater than 10 magnitudes.
Position(2000): RA = 19:05:12.5 Dec = +05:14:12.0 +/- 0.4".
[ur...
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V1174 Ori
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At this week's American Astronomical Society meeting in Minneapolis, Minnesota, Vanderbilt University astronomer Yilen Gómez Maqueo Chew and five colleagues presented detailed observations of the first known eclipsing binary system containing two brown dwarfs — star like gas balls not quit...
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Serpens SVS20
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Using the mid-infrared imager/spectrograph T-ReCS on the Gemini South telescope David Ciardi (Michelson Science Center, Caltech) and his collaborators have found that processing of dust grains around the proto-binary star Serpens SVS20 began at a surprisingly early point in...
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JW 451
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Low-Mass Runaway Stars from the Orion Trapezium Cluster
Authors: Arcadio Poveda, Christine Allen, Alejandro Hernandez-Alcantara
In the course of a search for common proper motion binaries, in the Jones & Walker (JW) catalogue of proper motions i...
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Hypernova GRB
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Hypernova Reveals Hidden Identity As Gamma-Ray Burst :
An international research team, led by astronomers from the University of Tokyo, Hiroshima University, and the National Astronomical Observatory of Japan, used the Subaru telescope to obtain the spectrum of SN2003jd...
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