Molecular-Hydrogen Absorption Features in the Spectrum of Quasi-Stellar Object 4c 05.34

1974 ◽  
Vol 190 ◽  
pp. L99 ◽  
Author(s):  
R. W. Carlson
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption ◽  
Stellar Object ◽  
Absorption Features

scholarly journals HST /COS SPECTRA OF DF Tau AND V4046 Sgr: FIRST DETECTION OF MOLECULAR HYDROGEN ABSORPTION AGAINST THE Lyα EMISSION LINE

2011 ◽  
Vol 730 (1) ◽  
pp. L10 ◽  
Author(s):  
Hao Yang ◽  
Jeffrey L. Linsky ◽  
Kevin France
Keyword(s):  
Emission Line ◽  
Molecular Hydrogen ◽  
Hydrogen Absorption

ON the Measurement and Interpretation of Absorption Features in the Spectrum of the Quasi-Stellar Object 3c 191

1966 ◽  
Vol 144 ◽  
pp. 447 ◽  
Author(s):  
E. M. Burbidge ◽  
C. R. Lynds ◽  
G. R. Burbidge
Keyword(s):  
Stellar Object ◽  
Absorption Features

scholarly journals Molecular hydrogen absorption systems in Sloan Digital Sky Survey

2014 ◽  
Vol 440 (1) ◽  
pp. 225-239 ◽  
Author(s):  
S. A. Balashev ◽  
V. V. Klimenko ◽  
A. V. Ivanchik ◽  
D. A. Varshalovich ◽  
P. Petitjean ◽  
...  
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption ◽  
Sloan Digital Sky Survey ◽  
Sky Survey

scholarly journals ANALYSIS OF MOLECULAR HYDROGEN ABSORPTION TOWARD QSO B0642–5038 FOR A VARYING PROTON-TO-ELECTRON MASS RATIO

2014 ◽  
Vol 782 (1) ◽  
pp. 10 ◽  
Author(s):  
J. Bagdonaite ◽  
W. Ubachs ◽  
M. T. Murphy ◽  
J. B. Whitmore
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption ◽  
Electron Mass ◽  
Mass Ratio

scholarly journals On determination of the cosmic ray flux using molecular hydrogen absorption lines

2003 ◽  
pp. 15-20
Author(s):  
Milan Cirkovic ◽  
I. Damjanov
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption ◽  
High Redshift ◽  
Cosmic Ray ◽  
Absorption Lines ◽  
High Mass ◽  
Proton Density ◽  
Mass Star ◽  
Cosmic Ray Flux

We outline a procedure for estimating the cosmic ray flux at remote locations where molecular hydrogen absorption lines have been detected. The method relies on several assumptions whose validity in the local Galactic ISM has been independently verified, so it might be useful for much less accessible objects, especially damped Ly? absorption systems. Since most of low-energy cosmic rays in the Galactic environment are thought to originate in supernovae remnants, the link to the rate of high-mass star formation could in principle, be established. We applied the method to a particular case of high redshift damped Ly? absorption system towards 0528?250 and obtained an estimate of proton density and some useful constraints.

scholarly journals The Secret Inner Life of the Orion Nebula

2001 ◽  
Vol 18 (1) ◽  
pp. 58-63
Author(s):  
A. S. B. Schultz
Keyword(s):  
Molecular Hydrogen ◽  
Stellar Object ◽  
Orion Nebula ◽  
Inner Life ◽  
Young Stellar Object

AbstractBeneath the familiar surface of the Orion Nebula is a spectacular molecular hydrogen outflow from a young stellar object, of very unusual morphology. In this paper I briefly discuss this outflow, its possible origins, and its interaction with the Nebula.

scholarly journals MOLECULAR HYDROGEN ABSORPTION FROM THE HALO OF Az∼ 0.4 GALAXY

2016 ◽  
Vol 823 (1) ◽  
pp. 66 ◽  
Author(s):  
Sowgat Muzahid ◽  
Glenn G. Kacprzak ◽  
Jane C. Charlton ◽  
Christopher W. Churchill
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption

scholarly journals Signatures of Hot Molecular Hydrogen Absorption from Protoplanetary Disks. I. Non-thermal Populations

2017 ◽  
Vol 846 (1) ◽  
pp. 6 ◽  
Author(s):  
Keri Hoadley ◽  
Kevin France ◽  
Nicole Arulanantham ◽  
R. O. Parke Loyd ◽  
Nicholas Kruczek
Keyword(s):  
Molecular Hydrogen ◽  
Hydrogen Absorption ◽  
Protoplanetary Disks
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