EXPORT: Spectral classification and projected rotational velocities of Vega-type and pre-main sequence stars

By A. Mora, B. Mer'in, E. Solano, B. Montesinos, D. D. Winter, C. Eiroa, R. Ferlet, C. Grady, J. Davies, L. F. Miranda and 12 more. 2001

173 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/04a73645504b4158c31a2accff527dd295694ecf

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In Astronomy and Astrophysics

1. M. Pecaut
2. Eric Mamajek
3. G. Herczeg
4. L. Hillenbrand
5. J. Monnier
6. Eric Bubar
7. A. Kraus
8. K. Luhman

Citations in the corpus

• A high-resolution spectropolarimetric survey of Herbig Ae/Be stars – I. Observations and measurements (2012, unknown): “…et al. (2004); (ar) Mora et al. (2004); (as) Fossati et al. (2009); (at) Miroshnichenko et al. (2004); (au) Hernández et al. (2005); (av) Bernabei et al. (2009); (aw) Hillenbrand et al. (1992); (ax) Mora et al. (2002); (ay) Mora et al. (2001); (az) Straižys, Černis & Bartašiūte (1996).”
• A spectroscopic survey of Herbig Ae/Be stars with X-shooter – I. Stellar parameters and accretion rates (2015, methodology): “…in this sample have had their stellar parameters determined previously, but this has often been done in smaller sub-sets using a variety of methods (Mora et al. 2001; Hernández et al. 2004; Manoj et al. 2006; Montesinos et al. 2009; Alecian et al. 2013, see also the Appendix for additional…”
• THE MASS DEPENDENCE BETWEEN PROTOPLANETARY DISKS AND THEIR STELLAR HOSTS (2013, unknown): “…White et al. (1999), 11 = Prato et al. (2002), 12 = Schaefer et al. (2012), 13 = Hartigan et al. (1994), 14 = Mathieu et al. (1997), 15 = White & Hillenbrand (2005), 16 = Dahm & Lyke (2011), 17 = Roberge et al. (2001), 18 = Massarotti et al. (2005), 19 = Mora et al. (2001), 20 = Gahm et al. (2008).”
• On the Interferometric Sizes of Young Stellar Objects (2002, background): “Note that for early spectral types the temperatures can be uncertain by thousands of Kelvin (e.g. MWC 297 has a 5 spectral subtype uncertainty; Mora et al. 2001).”
• AN OPTICAL SPECTROSCOPIC STUDY OF T TAURI STARS. I. PHOTOSPHERIC PROPERTIES (2014, background): “While RY Tau has had numerous spectral types bewteen F7–G1 Mora et al. (2001); Calvet et al. (2004); Hernandez et al. (2004), the Cohen & Kuhi (1979) spectral type of K1 has been adopted in several recent compulations.”
• C2D Spitzer-IRS spectra of disks around T Tauri stars. II. PAH emission features (2006, unknown): “…9: Dunkin et al. (1997), 10: Acke et al. (2005), 11: Assumed distance to Taurus-Auriga cloud (Kenyon et al. 1994), 12: Hernández et al. (2004), 13: Mora et al. (2001), 14: Straizys et al. (1996), 15: Finkenzeller & Mundt (1984), 16: Thé et al. (1994), 17: Houk (1978), 18: Alcala et al. (1995),…”
• A REVISED AGE FOR UPPER SCORPIUS AND THE STAR FORMATION HISTORY AMONG THE F-TYPE MEMBERS OF THE SCORPIUS–CENTAURUS OB ASSOCIATION (2011, methodology): “For the A8V standard, we adopt the star HD 158352 (HR 6507), which was classified as A8V by Cowley et al. (1969), Abt & Morrell (1995), and as A8Vp by Mora et al. (2001).”
• Few Skewed Disks Found in First Closure-Phase Survey of Herbig Ae/Be Stars (2006, background): “This star is variously spectral-typed as K1 (Akeson et al. 2005b) to F8 (Mora et al. 2001), an intermediate object between the Herbig Ae/Be and Classical T Tauri stars.”