Results 251 to 260 of about 190,834 (283)

Isolated osseous Rosai-Dorfman disease: a case report and review of literature. [PDF]

Skeletal Radiol
Sun JJ, Emert B, Dry S, Mofakham FA.
europepmc   +1 more source

Gene and genome duplications have contrasting impacts on biosynthetic and flower developmental pathways in California poppy. [PDF]

Plant Cell
Rössner LH, Rössner C, Kong D, Lotz D, Weisert A, Yamada Y, Sato F, Davies K, Rupp O, Fuchs J, Baldwin EA, Lovell J, McKain MR, Barry K, Bruna T, Talag J, Jenkins J, Walstead R, Grimwood J, Schmutz J, Leebens-Mack JH, Becker A.   +21 more
europepmc   +1 more source

The photometry and kinematics studies of NGC 2509 derived from Gaia DR3. [PDF]

Sci Rep
Ahmed NM, Tadross AL.
europepmc   +1 more source

Disseminated juvenile paracoccidioidomycosis: a case report and literature review. [PDF]

Einstein (Sao Paulo)
Ribeiro MES, Arouca LHNS, Ferreira JMG, Pasternak J, Curvelo LA, Matielo CEL.   +5 more
europepmc   +1 more source

Single-nucleus RNA-sequencing reveals the cellular programs driving nematode-induced giant cell formation in tomato. [PDF]

Hortic Res
Zadegan SB, Li P, Sultana MS, Abbas HMK, Coffey N, Öztürk C, Elwasif M, Rice JH, Krishnan HB, Hewezi T.   +9 more
europepmc   +1 more source

No evidence of mass segregation in massive young clusters [PDF]

Astronomy and Astrophysics, 2009
Aims. We investigate the validity of the mass segregation indicators commonly used in analysing young stellar clusters. Methods. We simulate observations by constructing synthetic seeing-limited images of a 1000 massive clusters (10^4 Msun) with a standard IMF and a King-density distribution function. Results.
João Alves
exaly   +4 more sources

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Young massive clusters in Arp 299

Proceedings of the International Astronomical Union, 2019
AbstractBecause of their young ages and compact densities, young massive star clusters (YMCs) are widely considered as potential proto-globular clusters. They are ubiquitous in environments with ongoing star formation activity such as interacting luminous infrared galaxies.
Zara Randriamanakoto, Petri Väisänen
openaire   +1 more source

Constraining globular cluster formation through studies of young massive clusters - II. A single stellar population young massive cluster in NGC 34 [PDF]

Monthly Notices of the Royal Astronomical Society, 2014
Currently there are two competing scenarios to explain the origin of the stellar population in globular clusters (GCs). The main difference between them is whether or not multiple events of star formation took place within GCs. In this paper we present the star formation history (SFH) of Cluster 1, a massive young cluster in NGC 34 $(\sim10^7\mbox{ M}_\
I Cabrera-Ziri, Nate Bastian, Gustavo Bruzual   +2 more
exaly   +3 more sources