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Results 11-20 of 32 (Search time: 0.004 seconds).
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Issue Date
Title
Author(s)
11-Dec-2014
A study of K i 7699 Å and related shell lines during the recent eclipse of ϵ Aurigae
Muthumariappan, C
;
Parthasarathy, M
;
Leadbeater, R
;
Potravnov, I. S
;
Appakutty, M
;
Jayakumar, K
1-Jul-2012
A Study of the Role of Lyβ Fluorescence on O I Line Strengths in Be Stars
Blesson, M
;
Banerjee, D. P. K
;
Subramaniam, A
;
Ashok, N. M
1-Dec-2013
Reappearance of McNeil’s Nebula (V1647 Orionis) and its Outburst Environment
Ninan, J. P
;
Ojha, D. K
;
Bhatt, B. C
;
Ghosh, S. K
;
Mohan, V
;
Mallick, K. K
;
Tamura, M
;
Henning, T
1-Sep-2013
The Progenitor of SN 2011ja: Clues from Circumstellar Interaction
Chakraborti, S
;
Ray, A
;
Smith, R
;
Ryder, S
;
Yadav, N
;
Sutaria, F. K
;
Dwarkadas, V. V
;
Chandra, P
;
Pooley, D
;
Roy, R
20-Aug-2013
Dust Around R Coronae Borealis Stars. II. Infrared Emission Features in an H-poor Environment
Garcia-Hernandez, D. A
;
Kameswara Rao, N
;
Lambert, D. L
11-Apr-2016
Physical parameters and long-term photometric variability of V1481 Ori, an SB2 member of Orion nebula Cluster with an accreting component
Messina, S
;
Parihar, P. S
;
Biazzo, K
;
Lanza, A. F
;
Distefano, E
;
Melo, C. H. F
;
Bradstreet, D. H
;
Herbst, W
May-2016
Spectroscopic study of Be-shell stars : 4 Her and 88 Her
Bhat, S. S
;
Paul, K. T
;
Subramaniam, A
;
Mathew, B
May-2017
The Curious Case of PDS 11: A Nearby, >10 Myr Old, Classical T Tauri Binary System
Mathew, B
;
Manoj, P
;
Bhatt, B. C
;
Sahu, D. K
;
Maheswar, G
;
Muneer, S
May-2015
Far-infrared study of K giants in the solar neighborhood: connection between Li enrichment and mass-loss
Bharat Kumar, Y
;
Reddy, B. E
;
Muthumariappan, C
;
Zhao, G
Jan-2012
Chemical composition of a sample of candidate post-asymptotic giant branch stars
Sumangala Rao, S
;
Giridhar, S
;
Lambert, D. L
Discover
Author
8
Kameswara Rao, N
7
Lambert, D. L
5
Parthasarathy, M
4
Mathew, B
4
Muthumariappan, C
4
Paul, K. T
4
Subramaniam, A
3
Garcia-Hernandez, D. A
3
Maheswar, G
3
Manoj, P
.
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Subject
8
Infrared: stars
7
Techniques: spectroscopic
6
Stars: pre-main sequence
5
Stars: AGB and post-AGB
4
Dust, extinction
4
Stars: chemically peculiar
4
Stars: emission-line, Be
4
Stars: evolution
4
Stars: mass-loss
4
White dwarfs
.
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2010 - 2018
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1993 - 1999