Zobrazeno 1 - 10
of 90
pro vyhledávání: '"Thai, T T"'
Autor:
Goovaerts, I., Pello, R., Burgarella, D., Thai, T. T., Richard, J., Claeyssens, A., Tuan-Anh, P., Arango-Toro, R. C., Boogaard, L., Contini, T., Guo, Y., Langan, I., Laporte, N., Maseda, M.
Faint, star-forming galaxies likely play a dominant role in cosmic reionisation. Strides have been made in recent years to characterise these populations at high redshifts ($z>3$). Now for the first time, with JWST photometry beyond 1$\,\mu m$ in the
Externí odkaz:
http://arxiv.org/abs/2401.12289
Autor:
Kramarenko, I. G., Kerutt, J., Verhamme, A., Oesch, P. A., Barrufet, L., Matthee, J., Kusakabe, H., Goovaerts, I., Thai, T. T.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 4, February 2024, Pages 9853-9871
The physical conditions giving rise to high escape fractions of ionizing radiation (LyC $f_{\rm{esc}}$) in star-forming galaxies - most likely protagonists of cosmic reionization - are not yet fully understood. Using the VLT/MUSE observations of ~140
Externí odkaz:
http://arxiv.org/abs/2305.07044
Autor:
Darriulat, P., Hoai, D. T., Nhung, P. T., Diep, P. N., Ngoc, N. B., Thai, T. T., Tuan-Anh, P.
The commonly accepted mechanism governing the formation of the nascent wind in oxygen-rich AGB stars combines an initial boost above the photosphere, given by shock waves resulting from stellar pulsations and convective cell granulation, with a subse
Externí odkaz:
http://arxiv.org/abs/2304.02837
Autor:
Nhung, P. T., Hoai, D. T., Darriulat, P., Diep, P. N., Ngoc, N. B., Thai, T. T., Tuan-Anh, P.
Publikováno v:
Research in Astronomy and Astrophysics (2024) Vol. 24, No. 3, id. 035009
New analyses of earlier ALMA observations of oxygen-rich AGB star EP Aquarii are presented, which contribute major progress to our understanding of the morpho-kinematics of the circumstellar envelope (CSE). The birth of the equatorial density enhance
Externí odkaz:
http://arxiv.org/abs/2304.01520
Autor:
Hoai, D. T., Nhung, P. T., Tan, M. N., Darriulat, P., Diep, P. N., Ngoc, N. B., Thai, T. T., Tuan-Anh, P.
The morpho-kinematics of the circumstellar envelope of oxygen-rich AGB star R Leonis is probed using ALMA (Atacama Large Millimeter/submillimeter Array) observations of the emission of molecular lines, including in particular CO(2-1) and $^{29}$SiO(5
Externí odkaz:
http://arxiv.org/abs/2211.02207
Autor:
Nhung, P. T., Hoai, D. T., Darriulat, P., Diep, P. N., Ngoc, N. T. B., Thai, T. T., Tuan-Anh, P
We use archival ALMA observations of the CO(2-1) and SiO(5-4) molecular line emissions of AGB star R Hya to illustrate the relative contributions of rotation, expansion and line broadening to the morphology and kinematics of the circumstellar envelop
Externí odkaz:
http://arxiv.org/abs/2207.06690
Autor:
Claeyssens, A., Richard, J., Blaizot, J., Garel, T., Kusakabe, H., Bacon, R., Bauer, F. E., Guaita, L., Jeanneau, A., Lagattuta, D., Leclercq, F., Maseda, M., Matthee, J., Nanayakkara, T., Pello, R., Thai, T. T., Tuan-Anh, P., Verhamme, A., Vitte, E., Wisotzki, L.
We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (-23
Externí odkaz:
http://arxiv.org/abs/2201.04674
Autor:
Hoai, D. T., Nhung, P. T., Darriulat, P., Diep, P. N., Ngoc, N. B., Thai, T. T., Tuan-Anh, P.
Single dish observations of AGB star L$_2$ Pup have revealed exceptionally low mass loss rate and expansion velocity, challenging interpretations in terms of standard wind models. Recent VLT and ALMA observations have drawn a detailed picture of the
Externí odkaz:
http://arxiv.org/abs/2111.13303
Autor:
Nhung, P. T., Hoai, D. T., Tuan-Anh, P., Darriulat, P., Diep, P. N., Ngoc, N. B., Thai, T. T.
Publikováno v:
ApJ, 927, 169 (2022)
With the aim of unraveling the complexity of the morpho-kinematics of the circumstellar envelope (CSE) of Mira Ceti, we review, extend and in some cases revisit ALMA millimeter observations of the emission of the SiO(5-4) and CO(3-2) molecular lines.
Externí odkaz:
http://arxiv.org/abs/2109.10730
Autor:
Nhung, P. T., Hoai, D. T., Tuan-Anh, P., Darriulat, P., Diep, P. N., Ngoc, N. B., Phuong, N. T., Thai, T. T.
We analyse new ALMA observations of the $^{29}$SiO ($\nu$=0, $J$=8$-$7) and SO$_2$($\nu$=0, $34_{3,31}$$-$$34_{2,32}$) line emissions of the circumstellar envelope (CSE) of the oxygen-rich AGB star R Dor. With a spatial resolution of $\sim$2.3 au, th
Externí odkaz:
http://arxiv.org/abs/2101.05455