14 research outputs found
Student Recital (April 26, 2012)
Adagio and Allegro, Op. 70 / Robert Schumann Susan Blazejewski, viola
Prelude in C minor, BWV 847 / Johann Sebastian Bach Important Event, Op. 15, No. 6 / Robert Schumann Carl Hollant, piano
Sonatina for Trombone and Piano / Bryan Kelly Agitato Daniel Hatchfield, trombone Carl Hollant, piano
Suite No. 1 in E minor, BWV 996 / J. S. Bach Prelude Jeremy Place, guitar
Sonata in a minor, BWV 1013 / J. S. Bach Allemande Amethyst Lambert, flute
Pie Jesu from Requiem in D minor, Op. 48 / Gabriel Fauré Mi Choe, soprano
Sonata No. 3, Op. 1, No. 12, HWV 370 / George Frideric Handel arr. Sigurd Rascher Adagio Allegro Mackenzie Leahy, alto saxophone
Fantasia / Sylvius Leopold Weiss Nicholas Rice, guitarhttps://vc.bridgew.edu/student_concerts/1020/thumbnail.jp
CMZoom IV. Incipient High-Mass Star Formation Throughout the Central Molecular Zone
In this work, we constrain the star-forming properties of all possible sites
of incipient high-mass star formation in the Milky Way's Galactic Center. We
identify dense structures using the CMZoom 1.3mm dust continuum catalog of
objects with typical radii of 0.1pc, and measure their association with
tracers of high-mass star formation. We incorporate compact emission at 8, 21,
24, 25, and 70um from MSX, Spitzer, Herschel, and SOFIA, catalogued young
stellar objects, and water and methanol masers to characterize each source. We
find an incipient star formation rate (SFR) for the CMZ of ~0.08 Msun yr^{-1}
over the next few 10^5 yr. We calculate upper and lower limits on the CMZ's
incipient SFR of ~0.45 Msun yr^{-1} and ~0.05 Msun yr^{-1} respectively,
spanning between roughly equal to and several times greater than other
estimates of CMZ's recent SFR. Despite substantial uncertainties, our results
suggest the incipient SFR in the CMZ may be higher than previously estimated.
We find that the prevalence of star formation tracers does not correlate with
source volume density, but instead ~75% of high-mass star formation is found in
regions above a column density ratio (N_{SMA}/N_{Herschel}) of ~1.5. Finally,
we highlight the detection of ``atoll sources'', a reoccurring morphology of
cold dust encircling evolved infrared sources, possibly representing HII
regions in the process of destroying their envelopes.Comment: Accepted for publication in Ap
CMZoom: Survey Overview and First Data Release
We present an overview of the CMZoom survey and its first data release.
CMZoom is the first blind, high-resolution survey of the Central Molecular Zone
(CMZ; the inner 500 pc of the Milky Way) at wavelengths sensitive to the
pre-cursors of high-mass stars. CMZoom is a 500-hour Large Program on the
Submillimeter Array (SMA) that mapped at 1.3 mm all of the gas and dust in the
CMZ above a molecular hydrogen column density of 10^23 cm^-2 at a resolution of
~3" (0.1 pc). In this paper, we focus on the 1.3 mm dust continuum and its data
release, but also describe CMZoom spectral line data which will be released in
a forthcoming publication. While CMZoom detected many regions with rich and
complex substructure, its key result is an overall deficit in compact
substructures on 0.1 - 2 pc scales (the compact dense gas fraction: CDGF). In
comparison with clouds in the Galactic disk, the CDGF in the CMZ is
substantially lower, despite having much higher average column densities. CMZ
clouds with high CDGFs are well-known sites of active star formation. The
inability of most gas in the CMZ to form compact substructures is likely
responsible for the dearth of star formation in the CMZ, surprising considering
its high density. The factors responsible for the low CDGF are not yet
understood but are plausibly due to the extreme environment of the CMZ, having
far-reaching ramifications for our understanding of the star formation process
across the cosmos.Comment: Accepted for Publication in ApJ
CMZoom III: Spectral Line Data Release
We present an overview and data release of the spectral line component of the
SMA Large Program, \textit{CMZoom}. \textit{CMZoom} observed CO(2-1),
CO(2-1) and CO(2-1), three transitions of HCO, several
transitions of CHOH, two transitions of OCS and single transitions of SiO
and SO, within gas above a column density of N(H)\,cm
in the Central Molecular Zone (CMZ; inner few hundred pc of the Galaxy). We
extract spectra from all compact 1.3\,mm \emph{CMZoom} continuum sources and
fit line profiles to the spectra. We use the fit results from the HCO
3(0,3)-2(0,2) transition to determine the source kinematic properties. We find
\% of the total mass of \emph{CMZoom} sources have reliable
kinematics. Only four compact continuum sources are formally self-gravitating.
The remainder are consistent with being in hydrostatic equilibrium assuming
that they are confined by the high external pressure in the CMZ. Based on the
mass and density of virially bound sources, and assuming star formation occurs
within one free-fall time with a star formation efficiency of , we
place a lower limit on the future embedded star-formation rate of \,M\,yr. We find only two convincing proto-stellar
outflows, ruling out a previously undetected population of very massive,
actively accreting YSOs with strong outflows. Finally, despite having
sufficient sensitivity and resolution to detect high-velocity compact clouds
(HVCCs), which have been claimed as evidence for intermediate mass black holes
interacting with molecular gas clouds, we find no such objects across the large
survey area.Comment: 44 pages, 41 figure
Student Recital (April 1, 2011)
Fairest Isle from King Arthur, Z. 628 / Henry Purcell Stuart Cabral, counter tenor
Must the winter come so soon? / Samuel Barber Diane M. Card, alto
Four Short Narratives / Neal Corwell 1. Morning 3. Dusk Andrew Shaw, euphonium
Alma del Core / Antonio Caldara Alison Kenney, soprano
Sonata / Paul Hindemith Allegro moderato maestoso Daniel Hatchfield, trombonehttps://vc.bridgew.edu/student_concerts/1007/thumbnail.jp
Outstanding Student Recital & Awards Ceremony (Feb. 2012)
Improvisation and Caprice / Eugene Bozza Sean Every, alto saxophone
Morceau Symphonique, Op.88 / Alexander Guilmant Charles Sherwin, euphonium
Quia respexit / Johann Sebastian Bach from Magnificat, BWV 243 Stuart Cabral, countertenor
O Ma Lyre Immortelle from Sapho / Charles Gounod Diane Card, alto
Habanera from Carmen / George Bizet Diane Card, alto
Barcarolle (Belle nuit, ô nuit d\u27amour) / Jacques Offenbach Stuart Cabral, countertenor Diane Card, alto
Prelude, No. 4 / Heitor Villa-Lobos Nicholas Rice, guitar
Waltz in B minor, Op. 60, No. 2 / Frédéric Chopin Carl Hollant, piano
Variations on the Carnival of Venice / arr. Jean-Baptiste Arban Daniel Hatchfield, trombonehttps://vc.bridgew.edu/student_concerts/1001/thumbnail.jp
Student Recital: Daniel Hatchfield, Trombone (October 23, 2012)
Sonata No. 4 in G minor / Benedetto Marcello Adagio Allegro Largo Allegro
T-Bone Concerto / Johan de Meij Rare Medium Well done
Play “A” To Start / Matt Ahrens Daniel Hatchfield and Matt Ahrens World Premier
Night on Bald Mountain / Modest Mussorgsky arr. by Charles Small
Hungarian Dance No. 5, WoO1 / Johannes Brahms arr. by Robert Elkjer Roy Campbell, Jared Cowell, Peter Griffin, Daniel Hatchfield, Nathanial Karahalis, Kevin Kardel, Becca Patterson, Donald Running, Chuck Sherwin
Posaunenstadt! / Eric Ewazen Roy Campbell, Jared Cowell, Peter Griffin, Daniel Hatchfield, Nathaniel Karahalis, Kevin Kardel, Sage Lewis, Becca Patterson, Donald Running, Matt Ahrens, Chuck Sherwin, Kevin Torreshttps://vc.bridgew.edu/student_concerts/1026/thumbnail.jp
CMZoom. IV. Incipient High-mass Star Formation throughout the Central Molecular Zone
In this work, we constrain the star-forming properties of all possible sites of incipient high-mass star formation in the Milky Way’s Galactic Center. We identify dense structures using the CMZoom 1.3 mm dust continuum catalog of objects with typical radii of ∼0.1 pc, and measure their association with tracers of high-mass star formation. We incorporate compact emission at 8, 21, 24, 25, and 70 μ m from the Midcourse Space Experiment, Spitzer, Herschel, and SOFIA, cataloged young stellar objects, and water and methanol masers to characterize each source. We find an incipient star formation rate (SFR) for the Central Molecular Zone (CMZ) of ∼0.08 M _⊙ yr ^−1 over the next few 10 ^5 yr. We calculate upper and lower limits on the CMZ’s incipient SFR of ∼0.45 and ∼0.05 M _⊙ yr ^−1 ,respectively, spanning roughly equal to and several times greater than other estimates of CMZ’s recent SFR. Despite substantial uncertainties, our results suggest the incipient SFR in the CMZ may be higher than previously estimated. We find that the prevalence of star formation tracers does not correlate with source volume density, but instead ≳75% of high-mass star formation is found in regions above a column density ratio ( N _SMA / N _Herschel ) of ∼1.5. Finally, we highlight the detection of atoll sources , a reoccurring morphology of cold dust encircling evolved infrared sources, possibly representing H ii regions in the process of destroying their envelopes
Student Recital (April 15, 2011)
Two, As One, In Three / John LaPorta Interplay / J. LaPorta Daniel Hatchfield, trombone Andrew Shaw, euphonium
Suite No. 3 in C / Johann Sebastian Bach 1. Prelude Susan Blazejewski, viola
Piano Sonata No. 2, Op. 31 / Dianne Goolkasian Rahbee) 1. Allegro maestoso Kurumi Ueno, piano
Dank sei Dir, Herr / Georg Friedrich Handel If you’ve only got a moustache / Stephen Collins Foster Patrick McMahon, bass
Sonata for Flute / Paul Hindemith II. Sehr langsam Deidre Balunas, flute
Black is the Color of My True Love’s Hair / John Jacob Niles Noh-Kyung Park, soprano
Two Hues of Blue / Lenny Niehaus 1. Moderate Blues Sean Every, alto saxophone
Pieta, Signore / Alessandro Stradella Ave Maria / C. Gounod Joseph Steinkrauss, baritone
El Testamen de N’amelia / Miguel Llobet Ian Timpany, guitar
Vanilla Ice Cream / Jerry Bock Alison Kenney, soprano
Lied der Mignon, Op. 62 / Franz Schubert Katie Sprusansky, mezzo soprano
Oboe Concerto in C minor / Benedetto Marcello III. Allegro James-ace Thackston, soprano saxophone
Trio in C Major for Two Violins and Viola, Op. 87 / Ludwig Van Beethoven 1. Allegro Chelsea White, violin I Elizabeth Smith, violin II Carla Mason, violin III Gail Columbo, violin IV Susan Blazejewski, violahttps://vc.bridgew.edu/student_concerts/1008/thumbnail.jp