Buscar

Mostrando ítems 1-10 de 188

Chasing discs around O-type (proto)stars: ALMA evidence for an SiO disc and disc wind from G17.64+0.16

Maud L.T.; Cesaroni R.; Kumar M.S.N.; Van Der Tak F.F.S.; Allen V.; Hoare M.G.; Klaassen P.D.; Harsono D.; Hogerheijde M.R.; Sánchez-Monge A.; Schilke P.; Ahmadi A.; Beltrán M.T.; Beuther H.; Csengeri T.; Etoka S.; Fuller G.; Galván-Madrid R.; Goddi C.; Henning T.; Johnston K.G.; Kuiper R.; Lumsden S.; Moscadelli L.; Mottram J.C.; Peters T.; Rivilla V.M.; Testi L.; Vig S.; De Wit W.J.; Zinnecker H. (EDP Sciences, 2018)

Completing the protostellar luminosity function in Cygnus-X with SOFIA/FORCAST imaging

Cheng, Yingjie; Gutermuth, Robert A.; Offner, Stella S.R.; Heyer, Mark H.; Zinnecker, Hans; Megeath, S. Thomas; Pokhrel, Riwaj (Oxford University Press, 2022)

Resolved star formation in the metal-poor star-forming region Magellanic Bridge C

Kalari, Venu M.; Rubio López, Mónica; Saldaño, Hugo P.; Bolatto, Alberto D. (Oxford University Press, 2020)

Magellanic Bridge C (MB-C) is a metal-poor (similar to 1/5 Z(circle dot)) low-density star-forming region located 59 kpc away in the Magellanic Bridge, offering a resolved view of the star formation process in conditions ...

Are T Tauri stars gamma-ray emitters?

Valle, María Victoria del; Romero, Gustavo Esteban; Luque Escamilla, Pedro Luis; Martí, Josep; Sánchez Sutil, Juan Ramón (2011)

Gamma-rays from massive protostars

Romero, Gustavo Esteban; Araudo, Anabella Teresa; Bosch Ramon, Valenti; Paredes, Josep María (Astronomical Society of the Pacific, 2010-06)

Massive protostars have associated bipolar outflows with velocities of hundreds of km s-1. Such outflows produce strong shocks when interact with the ambient medium leading to regions of non-thermal radio emission. Under ...

Massive protostars as gamma-ray sources

Bosch Ramon, V.; Romero, Gustavo Esteban; Araudo, Anabella Teresa; Paredes, J. M. (2010)

Pillars of Creation among Destruction: Star Formation in Molecular Clouds near R136 in 30 Doradus

Kalari V.M.; Rubio M.; Elmegreen B.G.; Guzmán V.V.; Zinnecker H.; Herrera C.N. (Institute of Physics Publishing, 2018)

Distribution of Serpens South protostars revealed with ALMA

Plunkett, Adele L.; Fernandez Lopez, Manuel; Arce, Héctor G.; Busquet, Gemma; Mardones, Diego; Dunham, Michael M. (EDP Sciences, 2018-07)

Context. Clusters are common sites of star formation, whose members display varying degrees of mass segregation. The cause may be primordial or dynamical, or a combination both. If mass segregation were to be observed in ...

Distribution of Serpens South protostars revealed with ALMA

Plunkett, Adele; Fernández López, Manuel; Arce, Héctor; Busquet, Gemma; Vivanco Mardones, Diego; Dunham, Michael (EDP Sciences, 2018-07-03)

Offset Jets around Protostar HH-34 in Orion

NASA; Jet Propulsion Laboratory; California Institute of Technology (Spitzer Space Telescope, 2016)

1
2
3
4
. . .
19

Buscar

Filtros

Chasing discs around O-type (proto)stars: ALMA evidence for an SiO disc and disc wind from G17.64+0.16

Completing the protostellar luminosity function in Cygnus-X with SOFIA/FORCAST imaging

Resolved star formation in the metal-poor star-forming region Magellanic Bridge C

Are T Tauri stars gamma-ray emitters?

Gamma-rays from massive protostars

Massive protostars as gamma-ray sources

Pillars of Creation among Destruction: Star Formation in Molecular Clouds near R136 in 30 Doradus

Distribution of Serpens South protostars revealed with ALMA

Distribution of Serpens South protostars revealed with ALMA

Offset Jets around Protostar HH-34 in Orion