Zobrazeno 1 - 10
of 3 604
pro vyhledávání: '"Mayer, L."'
Autor:
Delorme, P., Chomez, A., Squicciarini, V., Janson, M., Flasseur, O., Schib, O., Gratton, R., Lagrange, A-M., Langlois, M., Mayer, L., Helled, R., Reïffert, S, Kiefer, F., Biller, B., Chauvin, G., Fontanive, C., Henning, Th., Kenworthy, M., Marleau, G-D., Mesa, D., Meyer, M. R., Mordasini, C., Ringqvist, S. C., Samland, M., Vigan, A., Viswanath, G.
Exoplanets form from circumstellar protoplanetary discs whose fundamental properties (notably their extent, composition, mass, temperature and lifetime) depend on the host star properties, such as their mass and luminosity. B-stars are among the most
Externí odkaz:
http://arxiv.org/abs/2409.18793
Autor:
Béthermin, M., Accard, C., Guillaume, C., Dessauges-Zavadsky, M., Ibar, E., Cassata, P., Devereaux, T., Faisst, A., Freundlich, J., Jones, G. C., Kraljic, K., Algera, H., Amorin, R. O., Bardelli, S., Boquien, M., Buat, V., Donghia, E., Dubois, Y., Ferrara, A., Fudamoto, Y., Ginolfi, M., Guillard, P., Giavalisco, M., Gruppioni, C., Gururajan, G., Hathi, N., Hayward, C. C., Koekemoer, A. M., Lemaux, B. C., Magdis, G. E., Molina, J., Narayanan, D., Mayer, L., Pozzi, F., Rizzo, F., Romano, M., Tasca, L., Theulé, P., Vergani, D., Vallini, L., Zamorani, G., Zanella, A., Zucca, E.
The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density ($\Sigma_{\rm gas}$-$\Sigma_{\rm SFR}$) is essential to understand star formation processes in galaxies. So far, it has been measured up to z~2.5 in
Externí odkaz:
http://arxiv.org/abs/2311.08474
Autor:
Squicciarini, V., Gratton, R., Janson, M., Mamajek, E. E., Chauvin, G., Delorme, P., Langlois, M., Vigan, A., Ringqvist, S. C., Meeus, G., Reffert, S., Kenworthy, M., Meyer, M. R., Bonnefoy, M., Bonavita, M., Mesa, D., Samland, M., Desidera, S., D'Orazi, V., Engler, N., Alecian, E., Miglio, A., Henning, T., Quanz, S. P., Mayer, L., Flasseur, O., Marleau, G. D.
Publikováno v:
A&A 664, A9 (2022)
Virtually all known exoplanets reside around stars with $M<2.3~M_\odot$; to clarify if the dearth of planets around more massive stars is real, we launched the direct-imaging B-star Exoplanet Abundance STudy (BEAST) survey targeting B stars ($M>2.4~M
Externí odkaz:
http://arxiv.org/abs/2205.02279
Autor:
Lichtblau, M., Saxer, S., Müller, J., Appenzeller, P., Berlier, C., Schneider, S.R., Mayer, L., Furian, M., Schwarz, E.I., Swenson, E.R., Bloch, K.E., Ulrich, S.
Publikováno v:
In Pulmonology July-August 2024 30(4):362-369
Autor:
Sassano, F., Schneider, R., Valiante, R., Inayoshi, K., Chon, S., Omukai, K., Mayer, L., Capelo, P. R.
Observations of hyper-luminous quasars at $z>6$ reveal the rapid growth of supermassive black holes (SMBHs $>10^9 \rm M_{\odot}$) whose origin is still difficult to explain. Their progenitors may have formed as remnants of massive, metal free stars (
Externí odkaz:
http://arxiv.org/abs/2106.08330
Publikováno v:
A&A 652, L7 (2021)
The formation of the most massive quasars observed at high redshifts requires extreme inflows of gas down to the length scales of the central compact object. Here, we estimate the maximum inflow rate allowed by gravity down to the surface of supermas
Externí odkaz:
http://arxiv.org/abs/2105.13373
Autor:
Gallart, C., Monelli, M., Ruiz-Lara, T., Calamida, A., Cassisi, S., Cignoni, M., Anderson, J., Battaglia, G., Bermejo-Climent, J. R., Bernard, E. J., Martínez-Vázquez, C. E., Mayer, L., Salvadori, S., Monachesi, A., Navarro, J. F., Shen, S., Surot, F., Tosi, M., Bajaj, V., Strinfellow, G. S.
Eridanus II (EriII) is an ultra-faint dwarf (UFD) galaxy (M_V=-7.1) located at a distance close to the Milky Way virial radius. Early shallow color-magnitude diagrams (CMD) indicated that it possibly hosted an intermediate-age or even young stellar p
Externí odkaz:
http://arxiv.org/abs/2101.04464
Publikováno v:
In Environmental Modelling and Software January 2024 171
We investigated the formation and evolution of satellite systems in a cold, extended circumplanetary disc around a 10 $M_{\rm{Jupiter}}$ gas giant which was formed by gravitational instability at 50\,AU from its star. The disc parameters were from a
Externí odkaz:
http://arxiv.org/abs/1912.11406
Major mergers of gas-rich galaxies provide promising conditions for the formation of supermassive black holes (SMBHs; $\gtrsim10^5$ M$_\odot$) by direct collapse because they can trigger mass inflows as high as $10^4-10^5$ M$_\odot$ yr$^{-1}$ on sub-
Externí odkaz:
http://arxiv.org/abs/1910.04776