Results 221 to 229 of about 51,533 (229)

Identification of a putative new virus from the <i>Jingmenvirus</i> group in ticks from wild animals in Brazil. [PDF]

Virus Evol
Geraldini DB, Bittar C, Possebon FS, Gismene C, Mariutti RB, da Costa VG, Campos GRF, Beltrão RC, Neto GG, Lofego AC, Nogueira ML, Arni RK, Junior JPA, de Freitas Calmon M, Rahal P.   +14 more
europepmc   +1 more source

Simultaneous Liver Venous Deprivation Following Hepatic Arterial Chemoembolization Before Major Hepatectomy for Hepatocellular Carcinoma: A New Methods to Achieve Hypertrophy Liver Remnant. [PDF]

J Hepatocell Carcinoma
Zhang S, Song R, Hou C, Yao H, Xu J, Zhou H, Li S, Cai W, Fei Y, Meng F, Yin D, Wang J, Zhang S, Liu Y, Wang J, Liu L.   +15 more
europepmc   +1 more source

Activity-dependent refinement of axonal projections forms one-to-one connection pattern in the developing chick ciliary ganglion. [PDF]

Front Cell Neurosci
Egawa R, Yawo H, Kuba H.
europepmc   +1 more source

Loss of the cytosolic DNA-sensing genesCGASandSTING1in armadillos (Cingulata)

Schaffer L, Ivanoff A, Delsuc F, Lynch VJ.   +3 more
europepmc   +1 more source

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The Tip of the Red Giant Branch Distances to Typa Ia Supernova Host Galaxies. V. NGC 3021, NGC 3370, and NGC 1309 and the Value of the Hubble Constant

, 2017
We present final results of a program for the determination of the Hubble constant based on the calibration of the Type Ia supernovae (SNe Ia) using the Tip of the Red Giant Branch (TRGB).
I. Jang, M. Lee
semanticscholar   +1 more source

Carbon Abundances of M92 Red Giant Branch Stars

Publications of the Astronomical Society of the Pacific, 2001
Using CCD imaging, Fusi Pecci et al. have identified a local maximum at MV = -0.4 in the giant branch luminosity function of three co-added globular clusters having metallicities [Fe/H] ~ -2.2, including M92 (NGC 6341). Theories of deep mixing predict that surface carbon abundance depletions should be produced only within stars brighter than this ...
C. F. Claver, Susan Bellman, Graeme H. Smith, Michael M. Briley   +3 more
openaire   +2 more sources

Star Counts across the Red Giant Branch Bump and Below

The Astrophysical Journal, 2001
We present a new observable?Rbump?which is the ratio between the star counts across the red giant branch (RGB) bump and fainter RGB stars to investigate the occurrence of a deep-mixing phenomenon during these evolutionary phases. The comparison between predicted and empirical Rbump-values, based on a large and homogeneous set of Hubble Space Telescope ...
BONO G., CASSISI S., ZOCCALI M., PIOTTO, GIAMPAOLO   +3 more
openaire   +3 more sources

Evidence for non-standard mixing on the red giant branch

2008
Based on the new grid of standard stellar models computed at solar metallicity by the Geneva group (Schaller et al. 1992) with the recent OPAL opacity tables (Rogers & Iglesias 1992), we follow the theoretical evolution of the 12C/13C ratio along the red giant branch of low and intermediate mass stars.
openaire   +2 more sources

Lithium Rich Red Giant Branch Stars

2006
openaire   +2 more sources