The near-infrared spectra of low-mass X-ray binaries and related objects

1991 ◽  
Vol 373 ◽  
pp. 228 ◽  
Author(s):  
A. P. Cowley ◽  
P. C. Schmidtke ◽  
D. Crampton ◽  
J. B. Hutchings ◽  
M. Bolte
2020 ◽  
Vol 54 (5) ◽  
pp. 1151-1164 ◽  
Author(s):  
Ana Alves ◽  
Andrea Hevia ◽  
Rita Simões ◽  
Juan Majada ◽  
Ricardo Alia ◽  
...  

2013 ◽  
Vol 9 (S304) ◽  
pp. 195-198
Author(s):  
Angela Bongiorno

AbstractWe present new results on the the MBH-M∗ relation of X-ray obscured, red QSOs at high redshift (1.2<z<2.6). The sample is made of 21 red QSOs, nine of them are new sources for which near-infrared spectra have been obtained with SINFONI and XShooter observations at ESO VLT, and show a broad Hα component. The rest of the sample (12 sources) is made of sources taken from the literature with similar properties. From the broad Hα line we have computed the BH masses through the virial formula while stellar masses have been obtained through multi-component SED fitting.We find that red QSOs preferentially lie on the local relation up to z ~ 2.6 with the most massive objects mainly located above it. We also studied the evolution of these sources on the MBH-M∗ plane compared to a sample of optically blue type–1 QSOs and we find that obscured red QSOs show a constant MBH/M∗ ratio consistent/slightly higher than the local one but lower than what has been found for blue QSOs. These sources may represent the intermediate phase (blow-out phase) between the major-merger induced starbursts which appear as ULIRGs and SMGs and the optical type–1 blue QSOs which are revealed once the dust and nuclear gas is cleared up.


2007 ◽  
Vol 663 (2) ◽  
pp. 1215-1224 ◽  
Author(s):  
Cynthia S. Froning ◽  
Edward L. Robinson ◽  
Martin A. Bitner

2009 ◽  
Author(s):  
Dawn M. Gelino ◽  
Christopher R. Gelino ◽  
Thomas E. Harrison ◽  
Eric Stempels
Keyword(s):  
X Ray ◽  
Low Mass ◽  

2003 ◽  
Vol 211 ◽  
pp. 417-418
Author(s):  
Nadya Gorlova ◽  
Michael R. Meyer ◽  
Jim Liebert ◽  
George H. Rieke

We obtained near–infrared spectra of a sample of very low mass objects as a function of age in order to investigate the temperature and surface gravity sensitivity of several features in the J– and K–bands.


2012 ◽  
Vol 421 (4) ◽  
pp. 2846-2853 ◽  
Author(s):  
Mikhail G. Revnivtsev ◽  
Ivan Yu. Zolotukhin ◽  
Alexander V. Meshcheryakov
Keyword(s):  
X Ray ◽  
Low Mass ◽  

1988 ◽  
Vol 102 ◽  
pp. 47-50
Author(s):  
K. Masai ◽  
S. Hayakawa ◽  
F. Nagase

AbstractEmission mechanisms of the iron Kα-lines in X-ray binaries are discussed in relation with the characteristic temperature Txof continuum radiation thereof. The 6.7 keV line is ascribed to radiative recombination followed by cascades in a corona of ∼ 100 eV formed above the accretion disk. This mechanism is attained for Tx≲ 10 keV as observed for low mass X-ray binaries. The 6.4 keV line observed for binary X-ray pulsars with Tx&gt; 10 keV is likely due to fluorescence outside the He II ionization front.


2020 ◽  
Vol 16 ◽  
Author(s):  
Linqi Liu ◽  
JInhua Luo ◽  
Chenxi Zhao ◽  
Bingxue Zhang ◽  
Wei Fan ◽  
...  

BACKGROUND: Measuring medicinal compounds to evaluate their quality and efficacy has been recognized as a useful approach in treatment. Rhubarb anthraquinones compounds (mainly including aloe-emodin, rhein, emodin, chrysophanol and physcion) are its main effective components as purgating drug. In the current Chinese Pharmacopoeia, the total anthraquinones content is designated as its quantitative quality and control index while the content of each compound has not been specified. METHODS: On the basis of forty rhubarb samples, the correlation models between the near infrared spectra and UPLC analysis data were constructed using support vector machine (SVM) and partial least square (PLS) methods according to Kennard and Stone algorithm for dividing the calibration/prediction datasets. Good models mean they have high correlation coefficients (R2) and low root mean squared error of prediction (RMSEP) values. RESULTS: The models constructed by SVM have much better performance than those by PLS methods. The SVM models have high R2 of 0.8951, 0.9738, 0.9849, 0.9779, 0.9411 and 0.9862 that correspond to aloe-emodin, rhein, emodin, chrysophanol, physcion and total anthraquinones contents, respectively. The corresponding RMSEPs are 0.3592, 0.4182, 0.4508, 0.7121, 0.8365 and 1.7910, respectively. 75% of the predicted results have relative differences being lower than 10%. As for rhein and total anthraquinones, all of the predicted results have relative differences being lower than 10%. CONCLUSION: The nonlinear models constructed by SVM showed good performances with predicted values close to the experimental values. This can perform the rapid determination of the main medicinal ingredients in rhubarb medicinal materials.


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