Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Jang-Condell H"'
Autor:
Debes, J., Nealon, R., Alexander, R., Weinberger, A. J., Wolff, S. G., Hines, D., Kastner, J., Jang-Condell, H., Pinte, C., Plavchan, P., Pueyo, L.
Publikováno v:
The Astrophysical Journal 2003 948, 36
We report new total intensity visible light high contrast imaging of the TW Hya disk taken with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST). This represents the first published images of the disk with STIS sinc
Externí odkaz:
http://arxiv.org/abs/2305.03611
Autor:
D'Orazi, V., Gratton, R., Desidera, S., Avenhaus, H., Mesa, D., Stolker, T., Giro, E., Benatti, S., Jang-Condell, H., Rigliaco, E., Sissa, E., Scatolin, T., Benisty, M., Bhowmik, T., Boccaletti, A., Bonnefoy, M., Brandner, W., Buenzli, E., Chauvin, G., Daemgen, S., Damasso, M., Feldt, M., Galicher, R., Girard, J., Janson, M., Hagelberg, J., Mouillet, D., Kral, Q., Lannier, J., Lagrange, A. M., Langlois, M., Maire, A. -L., Menard, F., Moeller-Nilsson, O., Perrot, C., Peretti, S., Rabou, P., Ramos, J., Rodet, L., Roelfsema, R., Roux, A., Salter, G., Schlieder, J. E., Schmidt, T., Szulagyi, J., Thalmann, C., Thebault, P., van der Plas, G., Vigan, A., Zurlo, A.
For a comprehensive understanding of planetary formation and evolution, we need to investigate the environment in which planets form: circumstellar disks. Here we present high-contrast imaging observations of V4046 Sagittarii, a 20-Myr-old close bina
Externí odkaz:
http://arxiv.org/abs/1811.10621
We observe a significant change in the TW Hya disk interior to 40~AU via archival unpolarized multi-wavelength Hubble Space Telescope/STIS and NICMOS images with an inner working angle (IWA) of 0\farcs4 (22~AU). Our images show the outer edge of a cl
Externí odkaz:
http://arxiv.org/abs/1602.02090
We present a 0.5-2.2 micron scattered light spectrum of the circumstellar disk around TW Hya from a combination of spatially resolved HST STIS spectroscopy and NICMOS coronagraphic images of the disk. We investigate the morphology of the disk at dist
Externí odkaz:
http://arxiv.org/abs/1306.2969
Autor:
Grady, C. A., Muto, T., Hashimoto, J., Fukagawa, M., Currie, T., Biller, B., Thalmann, C., Sitko, M. L., Russell, R., Wisniewski, J., Dong, R., Kwon, J., Sai, S., Hornbeck, J., Schneider, G., Hines, D., Moro-Martin, A., Feldt, M., Henning, Th., Pott, J. -U., Bonnefoy, M., Bouwman, J., Lacour, S., Mueller, A., Juhasz, A., Crida, A., Chauvin, G., Andrews, S., Wilner, D., Kraus, A., Dahm, S., Robitaille, T., Jang-Condell, H., Abe, L., Akiyama, E., Brandner, W., Brandt, T., Carson, J., Egner, S., Follette, K. B., Goto, M., Guyon, O., Hayano, Y., Hayashi, M., Hayashi, S., Hodapp, K., Ishii, M., Iye, M., Janson, M., Kandori, R., Knapp, G., Kudo, T., Kusakabe, N., Kuzuhara, M., Mayama, S., McElwain, M., Matsuo, T., Miyama, S., Morino, J. -I., Nishimura, T., Pyo, T. -S., Serabyn, G., Suto, H., Suzuki, R., Takami, M., Takato, N., Terada, H., Tomono, D., Turner, E., Watanabe, M., Yamada, T., Takami, H., Usuda, T., Tamura, M.
We present the first near-IR scattered light detection of the transitional disk associated with the Herbig Ae star MWC 758 using data obtained as part of the Strategic Exploration of Exoplanets and Disks with Subaru, and 1.1 micron HST/NICMOS data. W
Externí odkaz:
http://arxiv.org/abs/1212.1466
Autor:
Berger, J. -P., Malbet, F., Baron, F., Chiavassa, A., Duvert, G., Elitzur, M., Freytag, B., Gueth, F., Hönig, S., Hron, J., Jang-Condell, H., Bouquin, J. -B. Le, Monin, J. -L, Monnier, J. D., Perrin, G., Plez, B., Ratzka, T., Renard, S., Stefl, S., Thiébaut, E., Tristram, K., Verhoelst, T., Wolf, S., Young, J.
The number of publications of aperture-synthesis images based on optical long-baseline interferometry measurements has recently increased due to easier access to visible and infrared interferometers. The interferometry technique has now reached a tec
Externí odkaz:
http://arxiv.org/abs/1204.4363
The $\gamma$ Cephei system is one of the most closely bound binary planet hosts known to date. The companion ($\gamma$ Cep B) to the planet-hosting star ($\gamma$ Cep A) should have truncated any protoplanetary disk around $\gamma$ Cep A, possibly li
Externí odkaz:
http://arxiv.org/abs/0807.4472
Autor:
Jang-Condell, H.
Planets embedded in optically thick passive accretion disks are expected to produce perturbations in the density and temperature structure of the disk. We calculate the magnitudes of these perturbations for a range of planet masses and distances. The
Externí odkaz:
http://arxiv.org/abs/0801.4561
Akademický článek
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Autor:
Worthen, K., Hom, J., Patience, J., Esposito, T., Duchene, G., Kalas, P., Jang-Condell, H., Saboi, K., Arriaga, P., Mazoyer, J., Wolff, S.G., Millar-Blanchaer, M., Fitzgerald, M., Perrin, M., Chen, C., Macintosh, B., Matthews, B., Wang, J., Graham, J., Marchis, F., Ammons, S., Bailey, V., Barman, T., Bulger, J., Chilcote, J., Cotten, T., Rosa, R..De., Doyon, R., Follette, K., Goodsell, S., Greenbaum, A., Hibon, P., Ingraham, P., Konopacky, Q., Larkin, J., Maire, J., Marley, M., Marois, C., Matthews, E., Metchev, S., Nielsen, E., Oppenheimer, R., Palmer, D., Poyneer, L., Pueyo, L., Rajan, A., Rameau, J., Rantakyro, F., Ren, B.
Publikováno v:
Bulletin of the American Astronomical Society, 143.03. AAS
ISSUE=3;STARTPAGE=143.03;TITLE=Bulletin of the American Astronomical Society
ISSUE=3;STARTPAGE=143.03;TITLE=Bulletin of the American Astronomical Society
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c0e341e764f202ecaebabec3c940525f
https://hdl.handle.net/1887/3142020
https://hdl.handle.net/1887/3142020