A study of the Keplerian accretion disk and precessing outflow in the massive protostar IRAS 20126+4104

By R. Cesaroni, R. Neri, L. Olmi, L. Testi, C. Walmsley, P. Hofner. 2005

140 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/f0c76567ec4b443bb86b262672d8dab8e77e7e42

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. D. Wilner
2. S. Andrews
3. A. Hughes
4. Th. Henning
5. C. Qi
6. T. Birnstiel
7. K. Rosenfeld
8. Jonathan P. Williams

In Spectroscopy

1. D. Wilner
2. S. Andrews
3. A. Hughes
4. C. Qi
5. K. Rosenfeld
6. Th. Henning
7. H. Klahr
8. R. Kuiper

Citations in the corpus

• Accretion disks in luminous young stellar objects (2015, background): “The prime examples for which this has been achieved are: IRAS 20126+4104 (Cesaroni et al., 2005), Cepheus A HW2 (Patel et al., 2005), G35.”
• A spectroscopic survey on the multiplicity of high-mass stars (2012, background): “Both observations of massive circumstellar disks (Shepherd, Claussen & Kurtz 2001; Chini et al. 2004; Cesaroni et al. 2005; Patel et al. 2005; Kraus et al. 2010) and theoretical calculations (Yorke & Sonnhalter 2002; Krumholz et al. 2009; Kuiper et al. 2010) seem to favour the accretion scenario.”
• Toward Understanding Massive Star Formation (2007, background): “…& Churchwell 1993) • Hot Star Workshop III: The Earliest Stages of Massive Star Birth (Crowther 2002) • Massive Star Birth: A Crossroads of Astrophysics (Cesaroni et al. 2005a) The reviews on Environment and Formation of Massive Stars (Garay & Lizano 1999), Control of Star Formation by Supersonic…”
• A SPATIALLY RESOLVED VERTICAL TEMPERATURE GRADIENT IN THE HD 163296 DISK (2013, background): “Furthermore, the contributions from the gas pressure gradient and self-gravity are model dependent, and so may become even more important for certain systems (e.g., Cesaroni et al. 2005; Bergin et al. 2013).”
• CIRCUMVENTING THE RADIATION PRESSURE BARRIER IN THE FORMATION OF MASSIVE STARS VIA DISK ACCRETION (2010, background): “Even circumstellar disks, e.g., IRAS 20126+4104 (Cesaroni et al. 1997; Zhang et al. 1998; Cesaroni et al. 2005) and AFGL 490 (Harvey et al. 1979; Torrelles et al. 1986; Chini et al. 1991; Davis et al. 1998; Lyder et al. 1998; Schreyer et al. 2002, 2006), or rather large-scale toroid (Beltrán et…”