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Results 1-10 of 11 (Search time: 0.004 seconds).
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Issue DateTitleAuthor(s)Citation
1995Ionized gas in the inner galaxyAnantharamaiah, K.R.; Lockman, F.J.; Kantharia, N.G.; Roshi, Anish D.Journal of Astrophysics and Astronomy Supplement, 1995, Vol. 16, p269-271.
2002A study of low density ionized gas in the galactic planeRoshi, Anish D.; Anantharamaiah, K.R.IAU Symposium, 2002, Vol.199, p335
2002Galactic carbon recombination lines near 327 MHzRoshi, Anish D.; Kantharia, N.G.; Anantharamaiah, K.R.IAU Symposium, 2002, Vol.199, p345
Nov-1997Hydrogen and carbon recombination lines towards the galactic centre near 328 MHzRoshi, Anish D.; Anantharamaiah, K.R.Monthly Notices of the Royal Astronomical Society, 1997, Vol.292, p63-70
Sep-2002Carbon recombination lines near 327 MHz. I. ``Diffuse'' C II regions in the Galactic DiskRoshi, Anish D.; Kantharia, N.G.; Anantharamaiah, K.R.Astronomy and Astrophysics, 2002, Vol.391, p1097-1113
20-May-2000Hydrogen recombination lines near 327 MHz. I. Distribution of low-density ionized gas in the galactic diskRoshi, Anish D.; Anantharamaiah, K.R.Astrophysical Journal, 2000, Vol.535, p231-246
2001Hydrogen recombination lines near 327 MHz - II: A galactic plane survey with a 2°x 6' beamRoshi, Anish D.; Anantharamaiah, K.R.Journal of Astrophysics and Astronomy, 2001, Vol.22, p81-119.
10-Aug-2001Hydrogen recombination lines near 327 MHz. III. Physical properties and origin of the low-density ionized gas in the inner galaxyRoshi, Anish D.; Anantharamaiah, K.R.Astrophysical Journal, 2001, Vol.557, p226-239
10-Jun-2005Multiwavelength carbon recombination line observations with the very large array toward an ultracompact H II region in W48: physical properties and kinematics of neutral materialRoshi, Anish D.; Goss, W.M.; Anantharamaiah, K.R.; Jeyakumar, S.Astrophysical Journal, 2005, Vol.626, p253-261
10-Jun-2006VLA observations of carbon 91α recombination line emission in W49 northRoshi, Anish D.; De Pree, C.G.; Goss, W.M.; Anantharamaiah, K.R.Astrophysical Journal, 2006, Vol.644, p279-282

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