Zobrazeno 1 - 10
of 223
pro vyhledávání: '"Paubert, G"'
Autor:
Torne, P., Macías-Pérez, J., Ladjelate, B., Ritacco, A., Sánchez-Portal, M., Berta, S., Paubert, G., Calvo, M., Desvignes, G., Karuppusamy, R., Navarro, S., John, D., Sánchez, S., Peñalver, J., Kramer, M., Schuster, K.
Publikováno v:
A&A 640, L2 (2020)
The investigation of pulsars between millimetre and optical wavelengths is challenging due to the faintness of the pulsar signals and the relative low sensitivity of the available facilities compared to 100-m class telescopes operating in the centime
Externí odkaz:
http://arxiv.org/abs/2007.02702
Autor:
Biver, N., Bockelée-Morvan, D., Paubert, G., Moreno, R., Crovisier, J., Boissier, J., Bertrand, E., Boussier, H., Kugel, F., McKay, A., Russo, N. Dello, DiSanti, M. A.
Publikováno v:
A&A 619, A127 (2018)
We present a multi-wavelength study of comet C/2016 R2 (PanSTARRS). This comet was observed on 23-24 January 2018 with the IRAM 30m telescope, and in January to March 2018 with the Nan\c{c}ay radio telescope. Visible spectroscopy was performed in Dec
Externí odkaz:
http://arxiv.org/abs/1809.08086
Publikováno v:
A&A 604, A12 (2017)
During the transition from the Asymptotic Giant Branch (AGB) to Planetary Nebulae (PN), the circumstellar geometry and morphology change dramatically. Another characteristic of this transition is the high mass loss rate, that can be partially explain
Externí odkaz:
http://arxiv.org/abs/1705.04588
Autor:
Torne, P., Desvignes, G., Eatough, R. P., Karuppusamy, R., Paubert, G., Kramer, M., Cognard, I., Champion, D. J., Spitler, L. G.
In Torne et al. (2015), we showed detections of SGR J1745-2900 up to 225 GHz (1.33 mm); at that time the highest radio frequency detection of pulsar emission. In this work, we present the results of new observations of the same magnetar with detectio
Externí odkaz:
http://arxiv.org/abs/1610.07616
Autor:
Biver, N., Moreno, R., Bockelée-Morvan, D., Sandqvist, Aa., Colom, P., Crovisier, J., Lis, D. C., Boissier, J., Debout, V., Paubert, G., Milam, S., Hjalmarson, A., Lundin, S., Karlsson, T., Battelino, M., Frisk, U., Murtagh, D., team, the Odin
Publikováno v:
A&A 589, A78 (2016)
The apparition of bright comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy) in March-April 2013 and January 2015, combined with the improved observational capabilities of submillimeter facilities, offered an opportunity to carry out sensitive composit
Externí odkaz:
http://arxiv.org/abs/1603.05006
Autor:
Torne, P., Eatough, R. P., Karuppusamy, R., Kramer, M., Paubert, G., Klein, B., Desvignes, G., Champion, D. J., Wiesemeyer, H., Kramer, C., Spitler, L. G., Thum, C., Güsten, R., Schuster, K. F., Cognard, I.
Publikováno v:
Torne P. et al., 2015, MNRAS, 451, L50
We report on simultaneous observations of the magnetar SGR J1745-2900 at frequencies $\nu = 2.54$ to $225\,\rm{GHz}$ using the Nancay 94-m equivalent, Effelsberg 100-m, and IRAM 30-m radio telescopes. We detect SGR J1745-2900 up to 225 GHz, the highe
Externí odkaz:
http://arxiv.org/abs/1504.07241
Autor:
Biver, N., Bockelée-Morvan, D., Debout, V., Crovisier, J., Boissier, J., Lis, D. C., Russo, N. Dello, Moreno, R., Colom, P., Paubert, G., Vervack, R., Weaver, H. A.
Publikováno v:
Astronomy & Astrophysics, 566, L5 (2014)
A spectral survey in the 1 mm wavelength range was undertaken in the long-period comets C/2012 F6 (Lemmon) and C/2013 R1 (Lovejoy) using the 30 m telescope of the Institut de radioastronomie millim\'etrique (IRAM) in April and November-December 2013.
Externí odkaz:
http://arxiv.org/abs/1405.6605
Autor:
Biver, N., Crovisier, J., Bockelée-Morvan, D., Szutowicz, S., Lis, D. C., Hartogh, P., de Val-Borro, M., Moreno, R., Boissier, J., Kidger, M., Küppers, M., Paubert, G., Russo, N. Dello, Vervack, R., Weaver, H., team, HssO
Publikováno v:
2012, Astron. Astrophys., 539, A68
The Jupiter-family comet 10P/Tempel 2 was observed during its 2010 return with the Herschel Space Observatory. We present here the observation of the (J, K) = (1, 0)-(0, 0) transition of ammonia at 572 GHz in this comet with the Heterodyne Instrument
Externí odkaz:
http://arxiv.org/abs/1201.4318
Autor:
Biver, N., Bockelée-Morvan, D., Colom, P., Crovisier, J., Paubert, G., Weiss, A., Wiesemeyer, H.
Publikováno v:
2011, Astronomy & Astrophysics, 528, A142
We present unique spectroscopic radio observations of comets C/2002 X5 (Kudo-Fujikawa), C/2002 V1 (NEAT), and C/2006 P1 (McNaught), which came within $r_h ~ 0.2 AU of the Sun in 2003 and 2007. The molecules OH, HCN, HNC, CS, and CH3OH were detected i
Externí odkaz:
http://arxiv.org/abs/1102.5015
Autor:
Biver, N., Bockelée-Morvan, D., Boissier, J., Crovisier, J., Colom, P., Lecacheux, A., Moreno, R., Paubert, G., Lis, D., Sumner, M., Frisk, U., Hjalmarson, A., Olberg, M., Winnberg, A., Florén, H. -G., Sandqvist, Aa., Kwok, Sun
Publikováno v:
Icarus 187: 253-271,2007
Comet 9P/Tempel 1 was the target of a multi-wavelength worldwide investigation in 2005. The NASA Deep Impact mission reached the comet on 4.24 July 2005, delivering a 370 kg impactor which hit the comet at 10.3 km/s. Following this impact, a cloud of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610717