Zobrazeno 1 - 10
of 10
pro vyhledávání: '"T. S. Barman"'
Autor:
Quinn M. Konopacky, T S. Barman
Publikováno v:
Handbook of Exoplanets ISBN: 9783319306483
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7163846f8e6a3b846e4f67794d5db6be
https://doi.org/10.1007/978-3-319-30648-3_36-1
https://doi.org/10.1007/978-3-319-30648-3_36-1
Publikováno v:
Proceedings of Indian National Science Academy, Vol 59, Iss 6B (2015)
Enhancement of Root Induction from In vitro Regenerated Shoots of Tea (Camellia sinensis L)
Autor:
J. K. Saikia, T. S. Barman
Publikováno v:
Photosynthetica. 43:283-287
Partitioning of 14C-labelled photosynthates to various parts of un-pruned tea clones TV1 and TV25 was assessed in vivo by exposing maintenance leaves to 14CO2 at monthly intervals throughout the year. The plants from shoot apex to root tip were divid
Autor:
J. I. Moses, M. R. Line, C. Visscher, M. R. Richardson, N. Nettelmann, J. J. Fortney, T. S. Barman, K. B. Stevenson, N. Madhusudhan
Publikováno v:
The Astrophysical journal, vol 777, iss 1
Neptune-sized extrasolar planets that orbit relatively close to their host stars -- often called "hot Neptunes" -- are common within the known population of exoplanets and planetary candidates. Similar to our own Uranus and Neptune, inefficient accre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf57316d6e7229842752b4c0871a76bf
http://arxiv.org/abs/1306.5178
http://arxiv.org/abs/1306.5178
Autor:
Q. M. Konopacky, A. M. Ghez, T. S. Barman, E. L. Rice, I. S. McLean, G. Duche^ne, Eric Stempels
Publikováno v:
AIP Conference Proceedings.
We present new dynamical mass estimates for a sample of brown dwarf binaries with sufficient precision (
Publikováno v:
AIP Conference Proceedings.
The physical conditions in a variety of objects (e.g. hot exoplanets and close binaries) are fundamentally influenced by external irradiation. In static cases this leads to the development of zones of different temperatures on the ‘day‐side’. I
Autor:
T. S. Barman
Water absorption is identified in the atmosphere of HD209458b by comparing models for the planet's transmitted spectrum to recent, multi-wavelength, eclipse-depth measurements (from 0.3 to 1 microns) published by Knutson et al. (2007). A cloud-free m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28a6cf4be61ae8cd56a63e63453a2330
http://arxiv.org/abs/0704.1114
http://arxiv.org/abs/0704.1114
Publikováno v:
Acta Horticulturae. :339-340
Autor:
J. I. Moses, M. S. Marley, K. Zahnle, M. R. Line, J. J. Fortney, T. S. Barman, C. Visscher, N. K. Lewis, M. J. Wolff
Publikováno v:
Astrophysical Journal; 10/1/2016, Vol. 829 Issue 2, p1-1, 1p
Autor:
Q. M. Konopacky, C. Marois, B. A. Macintosh, R. Galicher, T. S. Barman, S. A. Metchev, B. Zuckerman
Publikováno v:
Astronomical Journal; Aug2016, Vol. 152 Issue 2, p1-1, 1p