Zobrazeno 1 - 10
of 1 354
pro vyhledávání: '"Monsch A"'
Autor:
Guarcello, M. G., Almendros-Abad, V., Lovell, J. B., Monsch, K., Muzic, K., Martiinez-Galarza, J. R., Drake, J. J., Anastasopoulou, K., Andersen, M., Argiroffi, C., Bayo, A., Bonito, R., Capela, D., Damiani, F., Gennaro, M., Ginsburg, A., Grebel, E. K., Hora, J. L., Moraux, E., Najarro, F., Negueruela, I., Prisinzano, L., Richardson, N. D., Ritchie, B., Robberto, M., Rom, T., Sabbi, E., Sciortino, S., Umana, G., Winter, A., Wright, N. J., Zeidler, P.
The typically large distances, extinction, and crowding of Galactic supermassive star clusters have so far hampered the identification of their very low mass members, required to extend our understanding of star and planet formation, and early stella
Externí odkaz:
http://arxiv.org/abs/2411.13051
Autor:
Lovell, Joshua Bennett, Monsch, Kristina, Keating, Garrett K., Wilner, David J., Edenhofer, Gordian, Gurwell, Mark, Rao, Ramprasad
We present images of IRAS~08235--4316 with the Dark Energy Camera Plane Survey (DECaPS; spanning 0.398--1.034$\,\mu$m, at ${\sim}1''$ resolution) and the Submillimeter Array (SMA; at 1.38\,mm/217\,GHz, at ${\sim}1.9''\times1.2''$ resolution), a YSO l
Externí odkaz:
http://arxiv.org/abs/2411.10518
Autor:
Gossage, Seth, Kiman, Rocio, Monsch, Kristina, Medina, Amber A., Drake, Jeremy J., Garraffo, Cecilia, Yuxi, Lu, Wing, Joshua D., Wright, Nicholas J.
The relationship between magnetic activity and Rossby number is one way through which stellar dynamos can be understood. Using measured rotation rates and X-ray to bolometric luminosity ratios of an ensemble of stars, we derive empirical convective t
Externí odkaz:
http://arxiv.org/abs/2410.20000
Autor:
Monsch, Kristina, Lovell, Joshua B., Berghea, Ciprian T., Edenhofer, Gordian, Keating, Garrett K., Andrews, Sean M., Bayyari, Ammar, Drake, Jeremy J., Wilner, David J.
Publikováno v:
ApJL 967:L2 (9pp), 2024
We present resolved images of IRAS 23077+6707 ("Dracula's Chivito") in 1.3 mm/225 GHz thermal dust and CO gas emission with the Submillimeter Array (SMA) and optical (0.5-$0.8\,\mu\mathrm{m}$) scattered light with the Panoramic Survey Telescope and R
Externí odkaz:
http://arxiv.org/abs/2402.01941
Autor:
Cohen, Ofer, Glocer, Alex, Garraffo, Cecilia, Alvarado-Gomez, Julian, Drake, Jeremy, Monsch, Kristina, Puigdomenech, Farah Fauth
Exoplanets with short orbit period reside very close to their host stars. They transition very rapidly between different sectors of the circumstellar space environment along their orbit, leading to large variations of the magnetic field in the vicini
Externí odkaz:
http://arxiv.org/abs/2401.14459
The high-energy radiation emitted by young stars can have a strong influence on their rotational evolution at later stages. This is because internal photoevaporation is one of the major drivers of the dispersal of circumstellar disks, which surround
Externí odkaz:
http://arxiv.org/abs/2311.05673
Autor:
Drake, Jeremy J., Gomez, Julián Alvarado, Argiroffi, Costanza, Flaccomio, Ettore, Garraffo, Cecilia, Grosso, Nicolas, Islam, Nazma, Karovska, Margarita, Kashyap, Vinay L., Monsch, Kristina, Ness, Jan-Uwe, Sciortino, Salvatore, Wargelin, Bradford
We outline some of the highlights of the scientific case for the advancement of stellar high energy physics using the Line Emission Mapper X-ray Probe ({\it LEM}). The key to advancements with LEM lie in its large effective area -- up to 100 times th
Externí odkaz:
http://arxiv.org/abs/2310.17563
Autor:
Drake, Jeremy J., Cohen, David, Corcoran, Michael, Leutenegger, Maurice, Monsch, Kristina, Nazé, Yaël, Oskinova, Lidia, Antoniou, Vallia
We present some of the salient aspects of the scientific motivation for high resolution soft X-ray spectroscopy of early-type stars with the Line Emission Mapper X-ray Probe. The major strength of {\it LEM} for hot star physics is its large effective
Externí odkaz:
http://arxiv.org/abs/2310.16865
Photoevaporation from high energy stellar radiation has been thought to drive the dispersal of protoplanetary discs. Different theoretical models have been proposed, but their predictions diverge in terms of the rate and modality at which discs lose
Externí odkaz:
http://arxiv.org/abs/2308.12854
Autor:
Laura Gallucci, Christoph Sperber, Andreas U. Monsch, Stefan Klöppel, Marcel Arnold, Roza M. Umarova
Publikováno v:
Scientific Reports, Vol 14, Iss 1, Pp 1-9 (2024)
Abstract Given advantages in reperfusion therapy leading to mild stroke, less apparent cognitive deficits can be overseen in a routine neurological examination. Despite the widespread use of the Montreal Cognitive Assessment (MoCA), age- and educatio
Externí odkaz:
https://doaj.org/article/8726ff29b4ba44368796f2cd0cb99072
