Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Palau, Aina"'
Recent works have proposed the idea of a tidal screening scenario, in which tidal forces determine the mass that a protostar can accrete to explain the IMF. In this scenario, gravitationally unstable fragments will compete for the gas reservoir in a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::897ed60b4b9c774b802afd569df23394
http://arxiv.org/abs/2306.11106
http://arxiv.org/abs/2306.11106
Autor:
Yang, Dongting, Liu, Hong-Li, Tej, Anandmayee, Liu, Tie, Sanhueza, Patricio, Qin, Sheng-Li, Lu, Xing, Wang, Ke, Pan, Sirong, Xu, Feng-Wei, Vazquez-Semadeni, Enrique, Li, Shanghuo, Gomez, Gilberto C., Palau, Aina, Garay, Guido, Goldsmith, Paul F., Juvela, Mika, Saha, Anindya, Bronfman, Leonardo, Lee, Chang Won, Tatematsu, Kenichi, Dewangan, Lokesh, Zhou, Jianwen, Zhang, Yong, Stutz, Amelia, Eswaraiah, Chakali, Toth, L. Viktor, Ristorcelli, Isabelle, Shen, Xianjin, Luo, Anxu, Chibueze, James O.
There is growing evidence that high-mass star formation and hub-filament systems (HFS) are intricately linked. The gas kinematics along the filaments and the forming high-mass star(s) in the central hub are in excellent agreement with the new generat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf7e2af28a17bb342090191d7cb18578
http://arxiv.org/abs/2306.10332
http://arxiv.org/abs/2306.10332
Autor:
Li, Shanghuo, Lu, Xing, Zhang, Qizhou, Lee, Chang-Won, Sanhueza, Patricio, Beuther, Henrik, Izaskun, Jiménez-Serra, Qiu, Keping, Palau, Aina, Feng, Siyi, Pillai, Thushara, Kim, Kee-Tae, Liu, Hong-Li, Girart, Josep Miquel., Liu, Tie, Wang, Junzhi, Wang, Ke, Liu, Hauyu Baobab, Smith, Howard A., Li, Di, Lee, Jeong-Eun, Li, Fei, Li, Juan, Kim, Shinyoung, Yue, Nannan, Strom, Shaye
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Pre-stellar cores represent the initial conditions of star formation. Although these initial conditions in nearby low-mass star-forming regions have been investigated in detail, such initial conditions remain vastly unexplored for massive star-formin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4497831723441e488fcdc2d98d05d3e8
http://arxiv.org/abs/2104.05493
http://arxiv.org/abs/2104.05493
Autor:
Li, Shanghuo, Sanhueza, Patricio, Lee, Chang Won, Zhang, Qizhou, Beuther, Henrik, Palau, Aina, Liu, Hong-Li, Smith, Howard, Liu, Hauyu Baobab, Izaskun, Jim��nez-Serra, Kim, Kee-Tae, Feng, Siyi, Girart, Josep Miquel., Liu, Tie, Wang, Junzhi, Li, Di, Qiu, Keping, Lu, Xing, Wang, Ke, Li, Fei, Li, Juan, Cao, Yue, Kim, Shinyoung, Strom, Shaye
We present a study of narrow filaments toward a massive infrared dark cloud, NGC 6334S, using the Atacama Large Millimeter/submillimeter Array. Thirteen gas filaments are identified using the H13CO+ line, while a single continuum filament is revealed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::963306b50bed1a670be4c9cc7ebeaa12
Autor:
Zapata, Luis A., guez, Luis F. Rodr��, Fern��ndez-L��pez, Manuel, Palau, Aina, Estalella, Robert, Osorio, Mayra, Anglada, Guillem, Huelamo, Nuria
We present sensitive and high angular resolution ($\sim$0.2-0.3$''$) (sub)millimeter (230 and 345 GHz) continuum and CO(2$-$1)/CO(3$-$2) line archive observations of the disk star system in UX Tauri carried out with ALMA (The Atacama Large Millimeter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13a063f03aed7af4e413512d30486f70
http://arxiv.org/abs/2005.01652
http://arxiv.org/abs/2005.01652
Autor:
Palau, Aina, Li, Di, Juarez, Carmen, Chapman, Nicholas, Myers, Philip, Morales-Calderon, Maria, Barrado, David, Bouy, Herve, Rodriguez, Luis, Zapata, Luis, Rodríguez, Luis, Bouy, Hervé, Morales-Calderón, María, Juárez, Carmen
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 444:833-845
We report on Submillimeter Array observations of the 870 micron continuum and CO(3-2), 13CO(2-1) and C18O(2-1) line emission of a faint object, SMM2E, near the driving source of the HH797 outflow in the IC348 cluster. The continuum emission shows an
Autor:
Galv��n-Madrid, Roberto, Rodr��guez, Luis F., Liu, Hauyu B., Costigan, Gr��inne, Palau, Aina, Zapata, Luis A., Loinard, Laurent
There is increasing evidence that episodic accretion is a common phenomenon in Young Stellar Objects (YSOs). Recently, the source HOPS 383 in Orion was reported to have a $\times 35$ mid-infrared -- and bolometric -- luminosity increase between 2004
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64183a0321c89b6d07eb988e169154b9
http://arxiv.org/abs/1506.04466
http://arxiv.org/abs/1506.04466
Autor:
Fontani, F., Palau, Aina, Busquet, G., Isella, A., Estalella, R., Sanchez-Monge, A., Caselli, P., Zhang, Q.
The intermediate- to high-mass star-forming region IRAS 20343+4129 is an excellent laboratory to study the influence of high- and intermediate-mass young stellar objects on nearby starless dense cores, and investigate for possible implications in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a14a3fbc68683944928b1ec00fb2c476
Autor:
Palau, Aina, Sanchez-Monge, A., Busquet, G., Estalella, R., Zhang, Q., Ho, P. T. P., Beltran, M. T., Beuther, H.
We observed with the VLA, PdBI, and SMA the centimeter and millimeter continuum, N2H+(1-0), and CO(2-1) emission associated with a dusty cloud harboring a nascent cluster with intermediate-mass protostars. At centimeter wavelengths we found a strong
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7883f27029997ee29ea2a1d171f88e2