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Browsing by Subject Spectral line width
Showing results 1 to 14 of 14
| Issue Date | Title | Author(s) |
| 1987-02 | Chromospheric CA II K-line variations in the sun as a star over a solar cycle | Sivaraman, K. R; Singh, J; Bagare, S. P; Gupta, S. S |
| 1993-06-15 | The combined effect of partial redistribution and non-coherent electron scattering on polarized resonance line transfer | Nagendra, K. N; Rangarajan, K. E; Mohan Rao, D |
| 1990-06 | Equivalent widths of hydrogen Lyman alpha line in an expanding spherical atmosphere | Peraiah, A; Ingalgi, M. F |
| 1992-04 | EXOSAT observations of the broad-line radio galaxy 3C 382 | Ghosh, K. K; Soundararajaperumal, S |
| 1991-12 | H-alpha variability in the quiescent spectrum of the recurrent nova T Coronae Borealis | Anupama, G. C; Prabhu, T. P |
| 1993-05 | High resolution spectroscopy of the R Coronae Borealis star, V854 Centauri, during a deep minimum | Kameswara Rao, N; Lambert, D. L |
| 1988-03 | Is 21-cm absorption associated with the emission-line regions of quasars? | Krishan, V |
| 1991-05 | A new discussion on the M(v) - W(O I 7774 A) relationship for F-G stars in the light of high-resolution data | Arellano Ferro, A; Giridhar, S; Goswami, A |
| 1981 | Optical depth effects on the formation of spectral lines in rotating and expanding spherical atmospheres | Peraiah, A; Raghunath, G; Nagendra, K. N |
| 1987 | Polarization line radiative transfer in the atmospheres of magnetic white dwarfs | Nagendra, K. N |
| 1992-03 | Spatio-temporal fluctuations in He I 10830 A line parameters - Evidence for spicule formation | Venkatakrishnan, P; Jain, S. K; Singh, J; Recely, F; Livingston, W. C |
| 1990-05 | Spectroscopic studies of R CrB during light minima - Absorption spectrum | Kameswara Rao, N; Giridhar, S; Ashoka, B. N |
| 1992-04 | X-ray continuum with an iron emission line from the radio-quiet quasar PHL 909 | Ghosh, K. K; Soundararajaperumal, S |
| 1991-10 | X-ray spectrum (0.1-10 keV) of the broad line radio galaxy - 3C 390.3 | Ghosh, K. K; Sondararajaperumal, S |