Search Publications

Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451
DOI: 10.1038/nature10366 Bibcode: 2011Natur.476..425Z

Berger, E.; Frail, D. A.; Kulkarni, S. R. +24 more

Active galactic nuclei, which are powered by long-term accretion onto central supermassive black holes, produce relativistic jets with lifetimes of at least one million years, and the observation of the birth of such a jet is therefore unlikely. Transient accretion onto a supermassive black hole, for example through the tidal disruption of a stray…

2011 Nature
eHST 388
Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe
DOI: 10.1038/nature10646 Bibcode: 2011Natur.480..348L

Kulkarni, S. R.; Filippenko, Alexei V.; Cenko, S. Bradley +26 more

Type Ia supernovae are thought to result from a thermonuclear explosion of an accreting white dwarf in a binary system, but little is known of the precise nature of the companion star and the physical properties of the progenitor system. There are two classes of models: double-degenerate (involving two white dwarfs in a close binary system) and si…

2011 Nature
eHST 299
A candidate redshift z~10 galaxy and rapid changes in that population at an age of 500Myr
DOI: 10.1038/nature09717 Bibcode: 2011Natur.469..504B

Trenti, M.; Oesch, P. A.; Carollo, C. M. +9 more

Searches for very-high-redshift galaxies over the past decade have yielded a large sample of more than 6,000 galaxies existing just 900-2,000million years (Myr) after the Big Bang (redshifts 6>z>3 ref. 1). The Hubble Ultra Deep Field (HUDF09) data have yielded the first reliable detections of z~8 galaxies that, together with reports of a γ-r…

2011 Nature
eHST 294
An actively accreting massive black hole in the dwarf starburst galaxy Henize2-10
DOI: 10.1038/nature09724 Bibcode: 2011Natur.470...66R

Johnson, Kelsey E.; Reines, Amy E.; Sivakoff, Gregory R. +1 more

Supermassive black holes are now thought to lie at the heart of every giant galaxy with a spheroidal component, including our own Milky Way. The birth and growth of the first `seed' black holes in the earlier Universe, however, is observationally unconstrained and we are only beginning to piece together a scenario for their subsequent evolution. H…

2011 Nature
eHST 242
The unusual γ-ray burst GRB 101225A from a helium star/neutron star merger at redshift 0.33
DOI: 10.1038/nature10611 Bibcode: 2011Natur.480...72T

Im, M.; Fryer, C. L.; Choi, C. +31 more

Long γ-ray bursts (GRBs) are the most dramatic examples of massive stellar deaths, often associated with supernovae. They release ultra-relativistic jets, which produce non-thermal emission through synchrotron radiation as they interact with the surrounding medium. Here we report observations of the unusual GRB 101225A. Its γ-ray emission was exce…

2011 Nature
eHST 129
Supermassive black holes do not correlate with dark matter haloes of galaxies
DOI: 10.1038/nature09695 Bibcode: 2011Natur.469..377K

Kormendy, John; Bender, Ralf

Supermassive black holes have been detected in all galaxies that contain bulge components when the galaxies observed were close enough that the searches were feasible. Together with the observation that bigger black holes live in bigger bulges, this has led to the belief that black-hole growth and bulge formation regulate each other. That is, blac…

2011 Nature
eHST 128
A close nuclear black-hole pair in the spiral galaxy NGC3393
DOI: 10.1038/nature10364 Bibcode: 2011Natur.477..431F

Elvis, M.; Fabbiano, G.; Wang, Junfeng +1 more

The current picture of galaxy evolution advocates co-evolution of galaxies and their nuclear massive black holes, through accretion and galactic merging. Pairs of quasars, each with a massive black hole at the centre of its galaxy, have separations of 6,000 to 300,000 light years (refs 2 and 3; 1parsec = 3.26light years) and exemplify the first st…

2011 Nature
eHST 94
X-ray illumination of the ejecta of supernova 1987A
DOI: 10.1038/nature10090 Bibcode: 2011Natur.474..484L

Panagia, N.; Larsson, J.; Sollerman, J. +25 more

When a massive star explodes as a supernova, substantial amounts of radioactive elements--primarily 56Ni, 57Ni and 44Ti--are produced. After the initial flash of light from shock heating, the fading light emitted by the supernova is due to the decay of these elements. However, after decades, the energy powering a s…

2011 Nature
eHST 72
Black hole growth in the early Universe is self-regulated and largely hidden from view
DOI: 10.1038/nature10103 Bibcode: 2011Natur.474..356T

Schawinski, Kevin; Gawiser, Eric; Volonteri, Marta +2 more

The formation of the first massive objects in the infant Universe remains impossible to observe directly and yet it sets the stage for the subsequent evolution of galaxies. Although some black holes with masses more than 109 times that of the Sun have been detected in luminous quasars less than one billion years after the Big Bang, thes…

2011 Nature
eHST 70
A distortion of very-high-redshift galaxy number counts by gravitational lensing
DOI: 10.1038/nature09619 Bibcode: 2011Natur.469..181W

Yan, Haojing; Windhorst, Rogier A.; Mao, Shude +1 more

The observed number counts of high-redshift galaxy candidates have been used to build up a statistical description of star-forming activity at redshift z>~7, when galaxies reionized the Universe. Standard models predict that a high incidence of gravitational lensing will probably distort measurements of flux and number of these earliest galaxie…

2011 Nature
eHST 69