Zobrazeno 1 - 10
of 120
pro vyhledávání: '"Szucs, Laszlo"'
Autor:
Hunter, Todd R., Indebetouw, Remy, Brogan, Crystal L., Berry, Kristin, Chang, Chin-Shin, Francke, Harold, Geers, Vincent C., Gómez, Laura, Hibbard, John E., Humphreys, Elizabeth M., Kent, Brian R., Kepley, Amanda A., Kunneriath, Devaky, Lipnicky, Andrew, Loomis, Ryan A., Mason, Brian S., Masters, Joseph S., Maud, Luke T., Muders, Dirk, Sabater, Jose, Sugimoto, Kanako, Szűcs, László, Vasiliev, Eugene, Videla, Liza, Villard, Eric, Williams, Stewart J., Xue, Rui, Yoon, Ilsang
Publikováno v:
Publications of the Astronomical Society of the Pacific, volume 135, number 1049, 074501, 2023 July 24
We describe the calibration and imaging heuristics developed and deployed in the ALMA interferometric data processing pipeline, as of ALMA Cycle 9. The pipeline software framework is written in Python, with each data reduction stage layered on top of
Externí odkaz:
http://arxiv.org/abs/2306.07420
Autor:
Long, Feng, Herczeg, Gregory J., Pascucci, Ilaria, Apai, Daniel, Henning, Thomas, Manara, Carlo F., Mulders, Gijs D., Szűcs, László., Hendler, Nathanial P.
ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate either different evolutionary paths of disks or different initial conditi
Externí odkaz:
http://arxiv.org/abs/1806.04826
Autor:
Tar, József, Varga, Bence, Galambos, Péter, Szűcs, László, Siket, Máté *, Varga, Árpád, Eigner, György *, Kovács, Levente *
Publikováno v:
In IFAC PapersOnLine 2022 55(17):230-235
We present numerical simulations of molecular clouds (MCs) with self-consistent CO gas-phase and isotope chemistry in various environments. The simulations are post-processed with a line radiative transfer code to obtain $^{12}$CO and $^{13}$CO emiss
Externí odkaz:
http://arxiv.org/abs/1604.04545
Autor:
Kóspál, Ágnes, Ábrahám, Péter, Csengeri, Timea, Gorti, Uma, Henning, Thomas, Moór, Attila, Semenov, Dmitry A., Szűcs, László, Güsten, Rolf
EX Lupi-type objects (EXors) form a sub-class of T Tauri stars, defined by sudden sporadic flare-ups of 1-5 magnitudes at optical wavelengths. These eruptions are attributed to enhanced mass accretion from the circumstellar disk to the star, and may
Externí odkaz:
http://arxiv.org/abs/1603.02855
Publikováno v:
In IFAC PapersOnLine 2021 54(15):304-309
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 445, Issue 4, 2014, p.4055-4072
The $^{13}$CO molecule is often used as a column density tracer in regions where the $^{12}$CO emission saturates. The $^{13}$CO column density is then related to that of $^{12}$CO by a uniform isotopic ratio. A similar approximation is frequently us
Externí odkaz:
http://arxiv.org/abs/1403.4912
Autor:
Skemer, Andrew J., Close, Laird M., Szűcs, László, Apai, Dániel, Pascucci, Ilaria, Biller, Beth A.
(Abridged) Since the discovery of the first directly-imaged, planetary-mass object, 2MASS 1207 b, several works have sought to explain a disparity between its observed temperature and luminosity. Given its known age, distance, and spectral type, 2MAS
Externí odkaz:
http://arxiv.org/abs/1103.1880
Publikováno v:
Astrophysical Journal 720 (2010) 1668-1673
Previous studies suggest that the planet-forming disks around very-low-mass stars/brown dwarfs may be flatter than those around more massive stars, in contrast to model predictions of larger scale heights for gas-disks around lower-mass stars. We con
Externí odkaz:
http://arxiv.org/abs/1007.3703
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