Zobrazeno 1 - 10
of 435
pro vyhledávání: '"Wozniak H"'
Autor:
Boselli, A., Fossati, M., Ferrarese, L., Boissier, S., Consolandi, G., Longobardi, A., Amram, P., Balogh, M., Barmby, P., Boquien, M., Boulanger, F., Braine, J., Buat, V., Burgarella, D., Combes, F., Contini, T., Cortese, L., Cote, P., Cote, S., Cuillandre, J. C., Drissen, L., Epinat, B., Fumagalli, M., Gallagher, S., Gavazzi, G., Gomez-Lopez, J., Gwyn, S., Harris, W., Hensler, G., Koribalski, B., Marcelin, M., McConnachie, A., Miville-Deschenes, M. A., Navarro, J., Patton, D., Peng, E. W., Plana, H., Prantzos, N., Robert, C., Roediger, J., Roehlly, Y., Russeil, D., Salome, P., Sanchez-Janssen, R., Serra, P., Spekkens, K., Sun, M., Taylor, J., Tonnesen, S., Vollmer, B., Willis, J., Wozniak, H., Burdullis, T., Devost, D., Mahoney, B., Manset, N., Petric, A., Prunet, S., Withington, K.
Publikováno v:
A&A 614, A56 (2018)
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-band Halpha+[NII] imaging survey carried out with MegaCam at the Canada-France-Hawaii Telescope. The survey covers the whole Virgo cluster region from its core to
Externí odkaz:
http://arxiv.org/abs/1802.02829
Autor:
van der Laan, T. P. R., Schinnerer, E., Emsellem, E., Meidt, S., Dumas, G., Boeker, T., Hunt, L., Haan, S., Mundell, C., Wozniak, H.
The distribution of gas in the central kiloparsec of a galaxy has a dynamically rapid evolution. Nonaxisymmetries in the gravitational potential of the galactic disk, such as a large scale stellar bar or spiral, can lead to significant radial motion
Externí odkaz:
http://arxiv.org/abs/1306.5758
Autor:
Madden, S. C., Ruyer, A. Remy, Galametz, M., Cormier, D., Lebouteiller, V., Galliano, F., Hony, S., Bendo, G. J., Smith, M. W. L., Pohlen, M., Roussel, H., Sauvage, M., Wu, R., Sturm, E., Poglitsch, A., Contursi, A., Doublier, V., Baes, M., Barlow, M. J., Boselli, A., Boquien, M., Carlson, L. R., Ciesla, L., Cooray, A., Cortese, L., De Looze, I., Irwin, J. A., Isaak, K., Kamenetzky, J., Karczewski, O. L., Lu, N., MacHattie, J. A., Halloran, B. O, Parkin, T. J., Rangwala, N., Schirm, M. R. P., Schulz, B., Spinoglio, L., Vaccari, M., Wilson, C. D., Wozniak, H.
The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies using 230h of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic observations of the Herschel Space Observatory and draws to this a rich database of a
Externí odkaz:
http://arxiv.org/abs/1305.2628
Autor:
Davies, J. I., Wilson, C. D., Auld, R., Baes, M., Barlow, M. J., Bendo, G. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Pohlen, M., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
Galactic cirrus emission at far-infrared wavelengths affects many extragalactic observations. Separating this emission from that associated with extragalactic objects is both important and difficult. In this paper we discuss a particular case, the M8
Externí odkaz:
http://arxiv.org/abs/1010.4770
We have recently identified a new radial migration mechanism resulting from the overlap of spiral and bar resonances in galactic disks. Here we confirm the efficiency of this mechanism in fully self-consistent, Tree-SPH simulations, as well as high-r
Externí odkaz:
http://arxiv.org/abs/1006.0484
Autor:
Pohlen, M., Cortese, L., Smith, M. W. L., Eales, S. A., Boselli, A., Bendo, G. J., Gomez, H. L., Papageorgiou, A., Auld, R., Baes, M., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Dwek, E., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeiliner, W. W.
By combining Herschel-SPIRE data with archival Spitzer, HI, and CO maps, we investigate the spatial distribution of gas and dust in the two famous grand-design spirals M99 and M100 in the Virgo cluster. Thanks to the unique resolution and sensitivity
Externí odkaz:
http://arxiv.org/abs/1005.5476
Autor:
Cortese, L., Bendo, G. J., Boselli, A., Davies, J. I., Gomez, H. L., Pohlen, M., Auld, R., Baes, M., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Dwek, E., Eales, S. A., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Srinivasan, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped a
Externí odkaz:
http://arxiv.org/abs/1005.2331
Autor:
O'Halloran, B., Galametz, M., Madden, S. C., Galliano, F., Hony, S., Sauvage, M., Pohlen, M., Bendo, G. J., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Isaak, K. G., Levenson, L. R., Lu, N., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Galaxy Survey guaranteed time Herschel Key Program. We confirm the presen
Externí odkaz:
http://arxiv.org/abs/1005.2091
Autor:
Eales, S. A., Smith, M. W. L., Wilson, C. D., Bendo, G. J., Cortese, L., Pohlen, M., Boselli, A., Gomez, H. L., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Davies, J. I., Dwek, E., Elbaz, D., Galametz, M., Galliano, F., Gear, W. K., Glenn, J., Griffin, M., Hony, S., Isaak, K. G., Levenson, L. R., Lu, N., Madden, S., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M. R. P., Spinoglio, L., Srinivasan, S., Stevens, J. A., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wozniak, H., Wright, G. S., Zeilinger, W. W.
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter,
Externí odkaz:
http://arxiv.org/abs/1005.2113
Autor:
Galametz, M., Madden, S. C., Galliano, F., Hony, S., Sauvage, M., Pohlen, M., Bendo, G. J., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Boselli, A., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., Cooray, A., Cormier, D., Cortese, L., Davies, J. I., Dwek, E., Eales, S. A., Elbaz, D., Gear, W. K., Glenn, J., Gomez, H. L., Griffin, M., Isaak, K. G., Levenson, L. R., Lu, N., O'Halloran, B., Okumura, K., Oliver, S., Page, M. J., Panuzzo, P., Papageorgiou, A., Parkin, T. J., Perez-Fournon, I., Rangwala, N., Rigby, E. E., Roussel, H., Rykala, A., Sacchi, N., Schulz, B., Schirm, M. R. P., Smith, M. W. L., Spinoglio, L., Stevens, J. A., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Vigroux, L., Wilson, C. D., Wozniak, H., Wright, G. S., Zeilinger, W. W.
We present the first Herschel PACS and SPIRE images of the low-metallicity galaxy NGC6822 observed from 70 to 500 mu and clearly resolve the HII regions with PACS and SPIRE. We find that the ratio 250/500 is dependent on the 24 mu surface brightness
Externí odkaz:
http://arxiv.org/abs/1005.1730