J/ApJ/930/16       Massive YSOs in the GC. II. IRTF spectra       (Jang+, 2022)

Massive young stellar objects in the Galactic center. II. Seeing through the ice-rich envelopes. Jang D., An D., Sellgren K., Ramirez S.V., Boogert A.C.A., Schultheis M. <Astrophys. J., 930, 16 (2022)> =2022ApJ...930...16J 2022ApJ...930...16J
ADC_Keywords: Galactic center; YSOs; Spectra, infrared; Spectral types; Extinction Keywords: Astrochemistry ; Galactic center ; Interstellar abundances ; Protostars ; Ice formation ; Young stellar objects Abstract: To study the demographics of interstellar ices in the Central Molecular Zone (CMZ) of the Milky Way, we obtain near-infrared spectra of 109 red point sources using NASA IRTF/SpeX at Maunakea. We select the sample from near- and mid-infrared photometry, including 12 objects in the previous paper of this series, to ensure that these sources trace a large amount of absorption through clouds in each line of sight. We find that most of the sample (100 objects) show CO band-head absorption at 2.3µm, tagging them as red (super-) giants. Despite the photospheric signature, however, a fraction of the sample with L-band spectra (9/82=0.11) exhibit large H2O ice column densities (N>2x1018cm-2), and six of them also reveal CH3OH ice absorption. As one of such objects is identified as a young stellar object (YSO) in our previous work, these ice-rich sight lines are likely associated with background stars in projection to an extended envelope of a YSO or a dense cloud core. The low frequency of such objects in the early stage of stellar evolution implies a low star-formation rate (≲0.02M/yr), reinforcing the previous claim on the suppressed star-formation activity in the CMZ. Our data also indicate that the strong "shoulder" CO2 ice absorption at 15.4µm observed in YSO candidates in the previous paper arises from CH3OH-rich ice grains having a large CO2 concentration [N(CO2)/N(CH3OH)∼1/3]. Description: We obtained 2-4um spectra for 109 red point-like sources using SpeX, a medium-resolution (R∼2000-2500) cross-dispersed spectrograph and imager at the 3.0m NASA Infrared Telescope Facility (IRTF) on Maunakea. For these objects that are potentially associated with the Central Molecular Zone (CMZ), we carried out observing runs on UT dates 2009-May-14--15 and 17, 2011-Jul-17--20, 2017-May-28--30, Jun-21--23, and Jul-23--24 to collect spectra for 11, 28, and 70 science targets in 2009, 2011, and 2017, respectively. See Section 2. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 58 109 IRTF/SpeX targets table3.dat 105 109 Parameter estimates from spectral fitting -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/295 : Spitzer IRAC survey of the galactic center (Ramirez+, 2008) II/316 : UKIDSS-DR6 Galactic Plane Survey (Lucas+ 2012) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) VIII/96 : 6-GHz methanol multibeam maser catalogue (Caswell+, 2010-12) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) J/ApJS/86/713 : IR spectroscopy of ices (Hudgins+, 1993) J/ApJS/91/347 : A 5-GHz VLA Survey of the Galactic Plane (Becker+ 1994) J/A+A/455/971 : Organic molecules in the Gal. center (Requena-Torres+, 2006) J/ApJ/670/1115 : IRS spectra at 38 positions in Gal. center (Simpson+, 2007) J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009) J/ApJS/181/227 : Catalog of 24um sources toward Galactic Center (Hinz+, 2009) J/A+A/495/157 : Interstellar extinction in Gal. Center (Schultheis+, 2009) J/ApJ/702/178 : YSOs in the central 400pc of the Galaxy (Yusef-Zadeh+, 2009) J/A+A/511/A18 : NIR observations of stars near SgrA* (Schoedel+, 2010) J/ApJ/736/133 : Spitzer-IRS study of massive YSOs in gal. center (An+, 2011) J/ApJ/737/73 : Infrared extinction toward the Gal. Centre (Fritz+, 2011) J/AJ/149/64 : MIPSGAL 24µm point source catalog (Gutermuth+, 2015) J/MNRAS/470/1462 : HOPS. III. Dense molecular gas properties (Longmore+, 2017) J/ApJ/857/59 : Spitzer/IRS observations of the Gal. Center (Simpson, 2018) J/A+A/642/A81 : APOGEE cool stars (Schultheis+, 2020) J/A+A/653/A133 : GALACTICNUCLEUS IV. JHKs imaging (Nogueras-Lara+, 2021) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- SSTGC SSTGC identifier 9- 24 A16 --- 2MASS 2MASS identifier (HHMMSSss+DDMMSSs; J2000) 26- 33 F8.4 deg GLON Galactic longitude 35- 41 F7.4 deg GLAT [-0.23/0.22] Galactic latitude 43- 53 A11 "Y/M/D" Date Observation date (UT) 55- 58 A4 --- Bands Bands ("K" or "K, L") -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- SSTGC SSTGC identifier 9- 12 F4.1 mag Av [9.5/67.6] Foreground visual extinction 14- 17 F4.1 mag e_Av [1.4/42] Av uncertainty 19- 33 A15 --- SpT Spectral type 35 A1 --- l_tau3.0 Limit flag on tau3.0 37- 40 F4.2 --- tau3.0 [0.01/4]? Optical depth of the 3um band from solid H2O (Section 3.2) 42- 45 F4.2 --- e_tau3.0 [0.01/1]? tau3.0 uncertainty 47 A1 --- l_tau3.4 Limit flag on tau3.4 49- 52 F4.2 --- tau3.4 [0.03/0.4]? Optical depth of the 3.4um hydrocarbon band (Section 3.3) 54- 57 F4.2 --- e_tau3.4 [0.01/0.2]? tau3.4 uncertainty 59 A1 --- l_tau3.54 Limit flag on tau3.54 61- 64 F4.2 --- tau3.54 [0.01/0.2]? Optical depth of the 3.54um from the CH3OH band (Section 3.4) 66- 69 F4.2 --- e_tau3.54 [0.01/0.1]? tau3.54 uncertainty 71 A1 --- l_NH2O Limit flag on NH2O 73- 76 F4.2 10+18cm-2 NH2O [0.01/6.4]? H2O column density 78- 81 F4.2 10+18cm-2 e_NH2O [0.02/1.6]? NH2O uncertainty 83 A1 --- l_NCH3OH Limit flag on NCH3OH 85- 88 F4.2 10+18cm-2 NCH3OH [0.02/0.6]? CH3OH column density 90- 93 F4.2 10+18cm-2 e_NCH3OH [0.02/0.2]? NCH3OH uncertainty 95- 99 A5 --- COabs CO absorption 101- 105 A5 --- Brgam Br γ emission -------------------------------------------------------------------------------- History: From electronic version of the journal References: An et al. Paper I. 2011ApJ...736..133A 2011ApJ...736..133A Cat. J/ApJ/736/133
(End) Emmanuelle Perret [CDS] 14-Mar-2024
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