Results 231 to 240 of about 51,041 (245)
An integrated mass drug administration against hymenolepiasis and schistosomiasis in Sudan. [PDF]
Jin Y.
europepmc +1 more source
Maize-Tripsacum-Teosinte allopolyploid (MTP), a novel dwarf mutant inducer tool in maize. [PDF]
Zhou Y+22 more
europepmc +1 more source
Assessing the impact of Krymsk 5, Piku 1 and Gisela 6 rootstocks on morphological and quality characteristics of sweet cherry. [PDF]
Ozturk B, Belen S, Aglar E.
europepmc +1 more source
Social and seasonal variation in dwarf mongoose home-range size, daily movements, and burrow use. [PDF]
Arbon JJ+4 more
europepmc +1 more source
Jan and mini-Jan, a model system for potato functional genomics. [PDF]
Xin H+8 more
europepmc +1 more source
White dwarfs sing the blues [PDF]
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]
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
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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
2011Based 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