Zobrazeno 1 - 10
of 33
pro vyhledávání: '"D. P. K. Banerjee"'
Autor:
D. P. K. Banerjee, C. E. Woodward, V. Joshi, A. Evans, F. M. Walter, G. H. Marion, E. Y. Hsiao, N. M. Ashok, R. D. Gehrz, S. Starrfield
Publikováno v:
The Astrophysical Journal Letters, Vol 954, Iss 1, p L16 (2023)
We report the detection of carbon monoxide (CO) and dust, formed under hostile conditions, in recurrent nova V745 Sco about 8.7 days after its 2014 outburst. The formation of molecules or dust has not been recorded previously in the ejecta of a recur
Externí odkaz:
https://doaj.org/article/9162686c2f9f48cfbcdcadc2fc37df52
Autor:
D. P. K. Banerjee, A. Evans, C. E. Woodward, S. Starrfield, K. Y. L. Su, N. M. Ashok, R. M. Wagner
Publikováno v:
The Astrophysical Journal Letters, Vol 952, Iss 2, p L26 (2023)
V445 Puppis, the only known Galactic helium nova, is a unique test bed to verify supernova (SN) theories in the single-degenerate channel that involve a white dwarf (WD) accreting matter from a helium-rich donor. An estimate of the mass of the helium
Externí odkaz:
https://doaj.org/article/8ecf0f17eafc4e3db7495bee7ef5ec7e
Autor:
A Evans, B Pimpanuwat, A M S Richards, D P K Banerjee, U Munari, M D Gray, B Hutawarakorn Kramer, A Kraus
Publikováno v:
Evans, A, Pimpanuwat, B, Richards, A M S, Banerjee, D P K, Munari, U, Gray, M D, Kramer, B H & Kraus, A 2022, ' Stringent limits on $^{28}$SiO maser emission from the recurrent nova T Coronae Borealis ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4, pp. 4894-4897 . https://doi.org/10.1093/mnras/stac1589
There are indications that the third known eruption of the recurrent nova T CrB is imminent, and multi-wavelength observations prior to the eruption are important to characterise the system before it erupts. T CrB is known to display the SiO fundamen
Autor:
B Kaminsky, A Evans, Ya V Pavlenko, C E Woodward, D P K Banerjee, R D Gehrz, F Walter, S Starrfield, I Ilyin, K G Strassmeier, R M Wagner
We present an analysis of the red giant component of the recurrent nova V3890 Sgr, using data obtained before and after its 2019 eruption. Its effective temperature is $T_{\rm eff}=3050\pm$200 K for $\log{g}=0.7$, although there are modest changes in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc5791ede7916af440418c947a98deb3
http://arxiv.org/abs/2207.14721
http://arxiv.org/abs/2207.14721
We present infrared spectroscopy of the 2019 eruption of the recurrent nova V3890 Sgr, obtained over the period 5.1-46.3 days after the eruption. The spectrum of the red giant became more prominent as the flux declined, and by day 46.3 dominated the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09aaf350fb0460211389509aee01a69c
Autor:
A Evans, Ya V Pavlenko, D P K Banerjee, U Munari, R D Gehrz, C E Woodward, S Starrfield, L A Helton, M Shahbandeh, S Davis, S Dallaporta, G Cherini
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:56-57
Autor:
E. Aydi, K. V. Sokolovsky, J. S. Bright, E. Tremou, M. M. Nyamai, A. Evans, J. Strader, L. Chomiuk, G. Myers, F-J. Hambsch, K. L. Page, D. A. H. Buckley, C. E. Woodward, F. M. Walter, P. Mróz, P. J. Vallely, T. R. Geballe, D. P. K. Banerjee, R. D. Gehrz, R. P. Fender, M. Gromadzki, A. Kawash, C. Knigge, K. Mukai, U. Munari, M. Orio, V. A. R. M. Ribeiro, J. L. Sokoloski, S. Starrfield, A. Udalski, P. A. Woudt
We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years after the classical nova event and lasted for more than 400 days, reaching
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e32bd2c37f5f238b5c05bf4de0f453f3
Autor:
N. M. Ashok, D. P. K. Banerjee
Publikováno v:
International Astronomical Union Colloquium. 175:468-471
The medium resolution (R=1000) near infrared spectra of 30 early type Be stars obtained during the period October 1998-April 1999 are presented. The Paschen β and Brackett γ lines are seen in emission in majority of these stars. The higher order Br
Autor:
N. M. Ashok, D. P. K. Banerjee
We present optical observations of the enigmatic nova-like variable V4332 Sgr. The importance of this object should not be understated since it is considered to be the possible prototype of a new class of eruptive variables. These objects have been t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f24e322ec5a59e7300a48b359b06265
Publikováno v:
Publications of the Astronomical Society of the Pacific. 104:1091
Velocity field mapping in extended astronomical sources like gaseous nebulae and galaxies as well as nebulosities surrounding certain stars is important to understand the relevant physical phenomena occurring in such objects. A seeing-limited imaging