J/MNRAS/453/976     Herbig Ae/Be X-shooter observations      (Fairlamb+, 2015)

A spectroscopic survey of Herbig Ae/Be stars with X-shooter. I. Stellar parameters and accretion rates. Fairlamb J.R., Oudmaijer R.D., Mendigutia I., Ilee J.D., van den Ancker M.E. <Mon. Not. R. Astron. Soc., 453, 976-1001 (2015)> =2015MNRAS.453..976F 2015MNRAS.453..976F (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Stars, pre-main sequence ; Spectroscopy ; Accretion Keywords: accretion, accretion discs - techniques: spectroscopic - stars: early-type - stars: formation - stars: pre-main-sequence - stars: variables: T Tauri, Herbig Ae/Be Abstract: Herbig Ae/Be stars (HAeBes) span a key mass range that links low- and high-mass stars, and thus provide an ideal window from which to explore their formation. This paper presents Very Large Telescope/X-shooter spectra of 91 HAeBes, the largest spectroscopic study of HAeBe accretion to date. A homogeneous approach to determining stellar parameters is undertaken for the majority of the sample. Measurements of the ultraviolet are modelled within the context of magnetospheric accretion, allowing a direct determination of mass accretion rates. Multiple correlations are observed across the sample between accretion and stellar properties: the youngest and often most massive stars are the strongest accretors, and there is an almost 1:1 relationship between the accretion luminosity and stellar luminosity. Despite these overall trends of increased accretion rates in HAeBes when compared to classical T Tauri stars, we also find noticeable differences in correlations when considering the Herbig Ae and Herbig Be subsets. This, combined with the difficulty in applying a magnetospheric accretion model to some of the Herbig Be stars, could suggest that another form of accretion may be occurring within Herbig Be mass range. Description: Observations were performed over a period of 6 months between 2009 October and 2010 April using the X-shooter echelle spectrograph, mounted at the VLT, Cerro Paranal, Chile. X-shooter provides spectra covering a large wavelength range of 3000-23000Å, split into three arms and taken simultaneously. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 97 91 List of observations table2.dat 138 91 Details of the derived stellar parameters table3.dat 107 91 Table of accretion rates tablea1.dat 65 91 Photometry from the literature refs.dat 83 51 References -------------------------------------------------------------------------------- See also: J/AJ/106/656 : Herbig Ae/Be stars (Brooke+, 1993) J/A+AS/104/315 : Member of Herbig Ae/Be stellar group (The+ 1994) J/A+AS/111/399 : Polarization variability in Herbig Ae/Be stars (Jain+, 1995) J/AJ/118/1043 : Herbig Ae/Be stars catalog (Herbst+, 1999) J/AJ/126/2971 : UBVRI photometry of 131 Herbig Ae/Be (Vieira+, 2003) J/AJ/129/856 : Herbig Ae/Be stars in nearby OB associations (Hernandez+ 2005) J/ApJ/653/657 : Spectroscopic observations of Herbig Ae/Be stars (Manoj+, 2006 J/ApJ/658/358 : Ae/Be stars of Magellanic Bridge in JHKs (Nishiyama+, 2007) J/ApJ/698/2031 : Polarimetry of HAeBe stars (Rodrigues+, 2009) J/A+A/555/A64 : Identifying gaps in flaring Herbig Ae/Be disks (Maaskant+, 2014) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Name 18- 19 I2 h RAh Right ascension (J2000) 21- 22 I2 min RAm Right ascension (J2000) 24- 27 F4.1 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination (J2000) 33- 34 I2 arcmin DEm Declination (J2000) 36- 39 F4.1 arcsec DEs Declination (J2000) 41- 50 A10 "date" Obs.date Observation date 52- 60 A9 --- TUVB UVB arm exposure time(s) (in seconds) 61- 69 A9 --- TVIS VIS arm exposure time(s) (in seconds) 71- 82 A12 --- TNIR NIR arm exposure time(s) (in seconds) 84- 85 I2 --- NDIT Number of detector integration times for the NIR arm 87- 89 I3 --- SNRUVB UBV arm signal-to-noise ratio 91- 93 I3 --- SNRVIS VIS arm signal-to-noise ratio 95- 97 I3 --- SNRNIR NIR arm signal-to-noise ratio -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Name 17- 21 I5 K Teff Effective temperature 23- 26 I4 K e_Teff rms uncertainty on Teff 28- 31 F4.2 [cm/s2] logg Surface gravity 33- 36 F4.2 [cm/s2] E_logg Error on logg (upper value) 38- 41 F4.2 [cm/s2] e_logg Error on logg (lower value) 43- 46 F4.2 [Lsun] logL Luminosity 48- 51 F4.2 [Lsun] E_logL Error on logL (upper value) 53- 56 F4.2 [Lsun] e_logL Error on logL (lower value) 58- 61 F4.1 Msun M Mass 63- 66 F4.1 Msun E_M Error on Mass (upper value) 68- 70 F3.1 Msun e_M Error on Mass (lower value) 72- 75 F4.1 Rsun R Radius 77- 79 F3.1 Rsun E_R Error on Radius (upper value) 81- 83 F3.1 Rsun e_R Error on Radius (lower value) 85- 88 F4.2 mag AV Absorption in V band 90- 93 F4.2 mag E_AV Error on AV (upper value) 95- 98 F4.2 mag e_AV Error on AV (lower value) 100-105 F6.2 Myr Age Age 107-112 F6.2 Myr E_Age Error on Age (upper value) 114-119 F6.2 Myr e_Age Error on Age (lower value) 121-124 I4 pc Dist Distance 126-129 I4 pc E_Dist Error on Distance (upper value) 131-134 I4 pc e_Dist Error on Distance (lower value) 136- 137 A2 --- Notes [+* ] Notes for stars for which a distance estimate from the literature is used, or if the star was moved to the ZAMS (1) 138 A1 --- r_Dist References for Dist (2) -------------------------------------------------------------------------------- Note (1): Notes as follows: + = A literature distance is initially adopted to these stars, as log(g) cannot be determined from the spectra alone * = Stars which have been placed on the ZAMS. Note (2): References as follows: a = de Zeeuw et al. (1999, Cat. J/AJ/117/354) b = van Leeuwen (2007A&A...474..653V 2007A&A...474..653V, Cat. I/311) c = Dahm & Simon (2005, Cat. J/AJ/129/829) d = Shevchenko et al. (1999, Cat. J/MNRAS/310/210) e = Ababakr et al. (2015MNRAS.452.2566A 2015MNRAS.452.2566A) f = Vieira et al. (2003, Cat. J/AJ/126/2971) g = Fukagawa et al. (2006ApJ...636L.153F 2006ApJ...636L.153F) h = Loinard et al. (2008ApJ...675L..29L 2008ApJ...675L..29L) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Name 18- 19 A2 --- l_DDB [=< ] Limit flag on DDB 20- 23 F4.2 mag DDB ?=- Measured Balmer excess 25- 28 F4.2 mag E_DDB ? Error on ΔDB (upper value) (1) 30- 33 F4.2 mag e_DDB ? Error on ΔDB (lower value) (1) 36- 37 A2 --- l_f [=< ] Limit flag on f 38- 41 F4.1 % f ?=- Filling factor 43- 46 F4.1 % E_f ? Error on f (upper value) 48- 51 F4.1 % e_f ? Error on f (lower value) 54- 55 A2 --- l_log(dMacc/dt) [=< ] Limit flag on log(dMacc/dt) 56- 61 F6.2 [Msun/yr] log(dMacc/dt) ?=- Derived accretion rate 63- 66 F4.2 [Msun/yr] E_log(dMacc/dt) ? Error on log(dMacc/dt) (upper value) 68- 71 F4.2 [Msun/yr] e_log(dMacc/dt) ? Error on log(dMacc/dt) (lower value) 73- 87 A15 --- Met Method(s) used to obtain the values 89- 90 A2 --- l_logLacc [=< ] Limit flag on logLacc 91- 95 F5.2 [Lsun] logLacc ?=- Accretion luminosity 97-100 F4.2 [Lsun] E_logLacc ? Error on logLacc (upper value) 102-105 F4.2 [Lsun] e_logLacc ? Error on logLacc (lower value) 107 A1 --- Note [y/n-] Achievable by MA (2) -------------------------------------------------------------------------------- Note (1): ΔDB errors are rounded to the closest 0.01 and include all systematic errors too. Note (2): notes which stars can have their excess modelled successfully by MA. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Namme 17- 21 F5.2 mag Umag U magnitude 23- 27 F5.2 mag Bmag B magnitude 29- 33 F5.2 mag Vmag V magnitude 35- 39 F5.2 mag Rmag ?=- R magnitude 41- 45 F5.2 mag Imag ?=- I magnitude 47 A1 --- r_Umag Reference for photometry, in refs.dat file 49- 53 I5 K Teffl Effective temperature 54 A1 --- n_Teffl [+] Note on Teff (1) 56- 57 A2 --- r_Teffl Reference for Teff, in refs.dat file 59- 62 I4 pc Distl ? Distance 64- 65 A2 --- r_Distl Reference for Distance, in refs.dat file -------------------------------------------------------------------------------- Note (1): + : These two stars are listed as objects QT3 (TYC 8581-2002-1) and QT4 (HD 114981) in the first table of Vieira et al. (2003, Cat. J/AJ/126/2971). However, their places appear swapped in the second table by these authors. This swap is supported by additional photometry of HD 114981 and by the authors' observed temperatures and the temperatures derived in this work. Based on this, we have swapped the photometry from Vieira et al. (2003, Cat. J/AJ/126/2971) around for these two stars. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- Ref Reference code 4- 22 A19 --- BibCode BibCode 24- 62 A39 --- Aut Author's name 64- 83 A20 --- Com Comments -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 15-Mar-2016
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