Bulletin of the Astronomical Society of India
V. S. Pawade1,D. K. Ojha2*,J. P. Ninan2, A. Tej3, B. C. Bhatt4, D. K. Sahu4,S. K. Ghosh2,S. S. Kaurav2,and V. Mohan5
1University of Mumbai, Kalina, Santacruz (E), Mumbai 400 098, India
2Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba,Mumbai 400 005, India
3Indian Institute of Space Science and Technology, Thiruvananthapuram 695 022,India
4Indian Institute of Astrophysics, Koramangala, Bangalore 560 034, India
5IUCAA,Post Bag 4, Ganeshkhind, Pune 411 007, India
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LDN 1415 nebula was first detected by Stecklum (2006)in early April 2006 in the vicinity of IRAS 04376+5413. In this paper, we present a study of the post-outburst phase of LDN 1415 nebula using optical (V;R; I) and near-infrared (J;H;K) photometric and low-resolution optical spectroscopic observations.
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Keywords :stars:formation stars:variables: other ISM:individual:(LDN 1415 nebula)