Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Wootten, H. A."'
Autor:
Marcelino, N., Gerin, M., Cernicharo, J., Fuente, A., Wootten, H. A., Chapillon, E., Pety, J., Lis, D. C., Roueff, E., Commerçon, B., Ciardi, A.
Publikováno v:
A&A 620, A80 (2018)
The Barnard 1b core shows signatures of being at the earliest stages of low-mass star formation, with two extremely young and deeply embedded protostellar objects. Hence, this core is an ideal target to study the structure and chemistry of the first
Externí odkaz:
http://arxiv.org/abs/1809.08014
Autor:
Gerin, M., Pety, J., Commercon, B., Fuente, A., Cernicharo, J., Marcelino, N., Ciardi, A., Lis, D. C., Roueff, E., Wootten, H. A., Chapillon, E.
The formation epoch of protostellar disks is debated because of the competing roles of rotation, turbulence, and magnetic fields in the early stages of low-mass star formation. Magnetohydrodynamics simulations of collapsing cores predict that rotatio
Externí odkaz:
http://arxiv.org/abs/1709.07702
Autor:
Fuente, Asunción, Gerin, Maryvonne, Pety, Jerome, Commercon, Benoit, Agúndez, Marcelino, Cernicharo, José, Marcelino, Nuria, Roueff, Evelyne, Lis, Darek C., Wootten, H. A.
The extremely young Class 0 object B1b-S and the first hydrostatic core (FSHC) candidate, B1b-N, provide a unique opportunity to study the chemical changes produced in the elusive transition from the prestellar core to the protostellar phase. We pres
Externí odkaz:
http://arxiv.org/abs/1709.00058
Autor:
Lis, D. C., Wootten, H. A., Gerin, M., Pagani, L., Roueff, E., van der Tak, F. F. S, Vastel, C., Walmsley, C. M.
We present Herschel, ALMA Compact Array (ACA), and Caltech Submillimeter Observatory (CSO) observations of the prestellar core in L1689N, which has been suggested to be interacting with a molecular outflow driven by the nearby solar type protostar IR
Externí odkaz:
http://arxiv.org/abs/1605.01239
Autor:
Favre, C., Wootten, H. A., Remijan, A. J., Brouillet, N., Wilson, T. L., Deapois, D., Baudry, A.
We report the first sub-arc second (0.65$\arcsec$ $\times$ 0.51$\arcsec$) image of the dimethyl ether molecule, (CH$_{3}$)$_{2}$O, toward the Orion Kleinmann-Low nebula (Orion--KL). The observations were carried at 43.4 GHz with the Expanded Very Lar
Externí odkaz:
http://arxiv.org/abs/1105.3204
Autor:
Shah, Ronak Y., Wootten, H. Alwyn
We report on a survey of \nh2d towards protostellar cores in low-mass star formation and quiescent regions in the Galaxy. Twenty-three out of thirty-two observed sources have significant ($\gsim 5\sigma$) \nh2d emission. Ion-molecule chemistry, which
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103264
We conducted VLA observations at 0".06 resolution of the 22 GHz water masers toward the Class 0 source S106 FIR (d=600 pc; 15" west of S106-IRS4) on two epochs separated by ~3 months. Two compact clusters of the maser spots were found in the center o
Externí odkaz:
http://arxiv.org/abs/astro-ph/9906495
Autor:
Marcelino, N., Gerin, M., Cernicharo, J., Fuente, A., Wootten, H. A., Chapillon, E., Pety, J., Lis, D. C., Roueff, E., Commercon, B., Ciardi, A.
Table B.2 contains the detected molecular transitions in the B1b-S protostar ordered by observed frequency. The table includes the molecule formula and transition, rest frequency, spectroscopic data, and line parameters obtained from Gaussian fits. (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_____10369::5d12b4f875588e7d538dc227fc1a15f1
https://hal.science/hal-01981359
https://hal.science/hal-01981359
Autor:
Gerin, M., Pety, J., Commerçon, B., Fuente, A., Cernicharo, J., Marcelino, N., Ciardi, A., Lis, D. C., Roueff, E., Wootten, H. A., Chapillon, E.
The data are provided as two separate FITS files, one for B1b-N and one for B1b-S. The data have been obtained with ALMA in continuum mode. Four continuum basebands with 2 GHz bandwidth, 128 channels each have been combined. Central sky frequencies o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_____10369::80ab4a79b42ee34d3efb2d6047835092
https://hal.science/hal-01617863
https://hal.science/hal-01617863
Autor:
Fuente, A., Gerin, M., Pety, J., Commerçon, B., Agúndez, Marcelino, Cernicharo, José, Marcelino, Nuria, Roueff, E., Lis, D.C., Wootten, H. A.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The extremely young Class 0 object B1b-S and the first hydrostatic core (FSHC) candidate, B1b-N, provide a unique opportunity to study the chemical changes produced in the elusive transition from the prestellar core to the protostellar phase. We pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0c7b96f3244e5da342756933ff4b39d2
http://hdl.handle.net/10261/188048
http://hdl.handle.net/10261/188048