Results 261 to 270 of about 4,030,490 (290)

Multi-omics and functional analysis of a bioengineered vascularized pancreatic cancer model reveal an immunosuppressive and therapy-resistant niche

Giustarini G, Kok Siong A, Kumar P, Teng G, Xi BKZ, Tan CX, Bhalla R, Kalaitsidou E, Tay A, Howland SW, Cappello P, Wu W, Chen J, Albani S, Adriani G.   +14 more
europepmc   +1 more source

Activation of transposable elements is linked to a region- and cell type-specific interferon response in Parkinson's disease. [PDF]

Sci Adv
Garza R, Adami A, Thiruvalluvan A, Wijesinghe S, Curle A, Tam O, Forcier T, Lagka DA, Kazakou NL, Atacho DAM, Sharma Y, Horvath V, Bermudez S, Johansson J, Rainbow DB, Castilla-Vallmanya L, Jones JL, Quaegebeur A, Hammell MG, Kirkeby A, Barker RA, Jakobsson J.   +21 more
europepmc   +1 more source

Genome analysis of <i>Neisseria gonorrhoeae</i> in Norway, 2016-2023, reveals shifting epidemiology in the wake of the COVID-19 pandemic. [PDF]

Microb Genom
Alfsnes K, Osnes MN, Gilboe HM, Eldholm V, Caugant DA.   +4 more
europepmc   +1 more source

Earth-mass planets with He atmospheres in the habitable zone of Sun-like stars. [PDF]

Nat Astron
Lammer H, Scherf M, Erkaev NV, Kubyshkina D, Gorbunova KD, Fossati L, Woitke P.   +6 more
europepmc   +1 more source

Young, Massive Star Clusters in the Antennae [PDF]

, 2008
While massive star clusters have been detected in almost every galaxy with appreciable star formation, they are most prevalent in interacting and merging galaxies. As many as 95% of these clusters will ultimately be disrupted, often in the first 10 Myr, but those clusters that do survive may be the progenitors of globular clusters.
Christopher, Micol Huw
openaire   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

Be stars in young clusters in the Magellanic Clouds

Space Science Reviews, 1993
A substantial fraction (typically 10%) of Galactic B stars consists of Be stars. While Galactic Be stars have been fairly well investigated, very little is known about the Be star content of the Magellanic Clouds (MCs). We present a refined method of Be star identification by CCD photometry and apply it to four young clusters and associations in the ...
Eva K. Grebel, Wm James Roberts, Jean-Marie Will, Klaas S. De Boer   +3 more
openaire   +1 more source

Most nearby young star clusters formed in three massive complexes [PDF]

Nature
Efforts to unveil the structure of the local interstellar medium and its recent star formation history have spanned the past seventy years. Recent studies utilizing precise data from space astrometry missions have revealed nearby, newly formed star ...
Núria Miret Roig, Sabine Reffert, Stefan Meingast   +2 more
exaly   +2 more sources

Search for B[e] Stars in Young Open Clusters

1998
The properties and the stellar content of five young open clusters have been investigated to identify new B[e] stars. After a detailed analysis we conclude that none of the ~ 260 relatively young early type stars can be identified as such. We propose that either the B[e] characteristic is not present in young stars or that due to the close proximity of
de Winter, D., van den Ancker, M.E., Perez, M.R.   +2 more
openaire   +2 more sources

The Young Star Clusters in S106

1994
Near-infrared imaging of a 10 × 10 arcmin region of the S106 molecular cloud reveals two embedded clusters coinciding with peaks in the CO emission. By counting foreground stars seen towards the molecular cloud, the distance to S106 is found to be 1.2±0.2 kpc. Assuming a theoretical mass-luminosity relationship for pre-main sequence stars, we find that
openaire   +1 more source

Relative content of Be stars in young open star clusters

Astronomy Letters, 2012
Based on high- and medium-resolution spectra, we analyze the population of Be stars in eight young open star clusters. We have found a clear dependence of the relative content of early-type (B0-B3) Be stars on the cluster age. The relative concentration of Be stars of spectral types B0–B3 gradually increases with cluster age, reaching its maximum value
A. E. Tarasov, S. L. Malchenko
openaire   +1 more source