Results 41 to 50 of about 1,628,489 (254)
Biophysical Profiling of Tumor Cell Lines [PDF]
Analytical Cellular Pathology, 2011 Despite significant differences in genetic profiles, cancer cells share common phenotypic properties, including membrane-associated changes that facilitate invasion and metastasis. The Corning Epic® optical biosensor was used to monitor dynamic mass rearrangements within and proximal to the cell membrane in tumor cell lines derived from cancers of the ...
Frederick Coffman +4 more
openaire +3 more sources
Data on Stark Broadening of Sn II Spectral Lines
DataData on spectral line widths and shifts broadened by interactions with charged particles, for 44 lines in the spectrum of ionized tin, for collisions with electrons and H II and HeII ions, are presented as online available tables.
Milan S. Dimitrijević +3 more
doaj +1 more source
Iron abundance determination for the solar-like stars HR 4345 and HR 6573 [PDF]
Serbian Astronomical Journal, 2004 Using the BLACKWELL software package written by R.O. Gray, the iron abundance of the solar-like stars HR 4345 and HR 6573 has been determined. The method is based on determination of the minimum dispersion (or the region of least confusion) of the iron ...
Vince Oliver I., Vince Ištvan I.
doaj +1 more source
A polar+equatorial wind model for broad absorption line quasars: I. Fitting the C IV BAL profiles
, 2010 Despite all the studies, the geometry of the wind at the origin of the blueshifted broad absorption lines (BAL) observed in nearly 20% of quasars still remains a matter of debate.
Arav +82 more
core +1 more source
Program of telluric lines monitoring [PDF]
Serbian Astronomical Journal, 2006 A new observational program of telluric lines monitoring was introduced at Belgrade Astronomical Observatory. The ultimate goal of this program is to investigate the properties of Earth’s atmosphere through modeling the observed profiles of telluric ...
Vince I. +5 more
doaj +1 more source
Synthetic Line Profiles for Pulsating Red Giants
, 2005 Pulsation influences atmospheric structures of variable AGB stars (Miras) considerably. Spectral lines of the CO dv=3 vibration-rotation bands (at 1.6mue) therefore have a very characteristic appearance in time series of high-resolution spectra.
Aringer, B. +5 more
core +3 more sources
Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Atoms, 2018 Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas.
Milan S. Dimitrijević +5 more
doaj +1 more source
Sensitivity of the MnI 539.47 nm spectral line to solar activity [PDF]
Serbian Astronomical Journal, 2004 CCD observations of the MnI 539.47 nm spectral line in the solar flux made at the Astronomical Observatory in Belgrade between 1994 and 2003 have been reduced and certain line parameters, viz.
Danilović Sanja, Vince Ištvan I.
doaj +1 more source
On resonance line profiles predicted by radiation driven disk wind models
, 2003 We report on resonance line profiles predicted by radiation driven disk wind models which extend radially one order of magnitude farther out than our previous models.
Beuermann K. +3 more
core +1 more source
Pediatric Blood &Cancer, EarlyView.ABSTRACT Pediatric gastroenteropancreatic neuroendocrine neoplasms (GEP‐NENs) are extremely rare and clinically heterogeneous. Management has largely been extrapolated from adult practice. This European Standard Clinical Practice Guideline (ESCP), developed by the EXPeRT network in collaboration with adult NEN experts, provides (adult) evidence ...
Michaela Kuhlen +23 more
wiley +1 more source