Results 231 to 240 of about 51,041 (245)

Maize-Tripsacum-Teosinte allopolyploid (MTP), a novel dwarf mutant inducer tool in maize. [PDF]

open access: yesPlant Biotechnol J
Zhou Y   +22 more
europepmc   +1 more source

Jan and mini-Jan, a model system for potato functional genomics. [PDF]

open access: yesPlant Biotechnol J
Xin H   +8 more
europepmc   +1 more source

INDETERMINATE DOMAIN-DELLA protein interactions orchestrate gibberellin-mediated cell elongation in wheat and barley

open access: yes
Sokolowska P   +13 more
europepmc   +1 more source

White dwarfs sing the blues [PDF]

open access: possibleNature, 1998
A new model predicts that the oldest white dwarf stars should look blue. That could help to identify what makes up the massive halo of our Galaxy, and to pin down the age of the Universe.
openaire   +1 more source

Isolated groups of extremely blue dwarf galaxies [PDF]

open access: possibleProceedings of the International Astronomical Union, 2019
AbstractInteractions and mergers between dwarf galaxies are mostly gas-rich and should be marked by an intense star formation activity. But these processes, which are expected to be common at earlier times, are very difficult to observe at low redshifts. To investigate that, we look in the Sloan Digital Sky Survey (SDSS) for compact groups that contain
Vitor Bootz   +5 more
openaire   +1 more source

Cometary Blue Compact Dwarf Galaxies

2001
‘Cometary’ Blue Compact Dwarf Galaxies (iI,C BCDs) are characterized by off-center starbursts close to the end of an elongated dwarf irregular (dI)-like host galaxy. This may either represent randomly enhanced star-forming activity of a dI, or may be caused by a set of special properties of such systems or their environment.
P. Papaderos   +5 more
openaire   +2 more sources

On the Metallicity of Blue Compact Dwarfs

2011
Based on the even distribution of metals in Blue Compact Dwarfs (BCDs) spread all over their volume, we show that a large amount of stars (≥108 M⊙) are required to justify such a homogeneous metal abundance. We also show that such a mass would imply a large number of bursts similar to the ones presently energizing the giant nebulae.
openaire   +2 more sources

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