Masers - Arcetri · Poster 41 on Serpens/Herschel by E. Fiorellino. Amazing bandwidth! The 32 meter...
Transcript of Masers - Arcetri · Poster 41 on Serpens/Herschel by E. Fiorellino. Amazing bandwidth! The 32 meter...
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Francesco’s Legacy Florence, 2017 June 7
Francesco and Francesco and MasersMasers
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Francesco’s Legacy Florence, 2017 June 7
Francesco and Francesco and MasersMasers
©F. Melandri
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Common Strong Interstellar Masers:
First found
Where Pump # known
OH Hydroxyl 1965 UCHIIRs R (FIR) many
H2O Water vapor
1969 L+HM YSOs
C very many
CH3OH Methanol 1971 (I) 1986 (II)
Class I outflowsClass II HMYSOs
Cl. I: C
Cl. II: R (FIR)
Class I: manyClass II: very many
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Genzel 1988
High n and high T
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t
H2O masers accretion powered/outflows
Class II CH3OH masers radiatively pumped need strong FIR field)
OH masers rad. pumped (FIR)
Rot. exc. OH absorption
Hot Cores
IRDC HCHIIR UCHIIR CHIIR
Masers in Regions of High Mass Star Formation
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The W3OH region – different stages of high-mass star formation
2
2) UCHII region: dynamical age 2300 yr VLA
Wilner, Reid, & Menten 1995
3
3) Even younger: Turner-Welch (1984) object
Compact dust/molecular hot core
1) CHII region: dynamical age ~ 5000 yr
1
OH and CH3 OH masers H
2O masers
Hachisuka+ 2006/VLBA
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W49 N
Cheung+ 1969
The 22.2 GHz H2O line•Discovered 1969 by Cheung … Townes …
• First triatomic interstellar molecule• In Orion, Sgr B2, W49 N• Very intense emission/ strongest
radio line: W 49 N ~ 1 L
•Level energies 643 K above ground•Very wide velocity spread•VLBI:
• Very compact, variable emission• Very high brightness temperaturesMaser• Collisonally pumped in post-J shock gas
Neufeld & Melnick 1991, Hollenbach+ 2013
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Zhang+ 2013/BeSSeL survey
H2O Maser motions in W49 N
Luminosity in 22.2 GHz H2O line ~1 L
Walker+ 1977
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Interstellar H2O Masers •are always associated with outflows trace accretion•are signposts for energy sources•Variability marks energetic events
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Interstellar H2O Masers •are always associated with outflows trace accretion•are signposts for energy sources•Variability marks energetic events
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Poster 41 on Serpens/Herschel by E. Fiorellino
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Amazing bandwidth!
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The 32 meter telescope of Medicina Radio Observatory•Built in 1983
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EVN – the European VLBI Network
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Marcello Felli
Gianni Tofani1938–2015
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(A somewhat later edition of) il gruppo radioastronomia di Arcetri
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(A somewhat later edition of) il gruppo radioastronomia di Arcetri
In 1986 the group started a spectroscopy program with the Medicina radio telescope. Digital autocorrelator built in Arcetri.
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1988
2001
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1992
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Friedrich Wilhelm Bessel (1748 –1846)
Medicina survey data provide targets
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VERA: VLBI Exploration of Radio Astronomy
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Reid+ 2014
Maser parallax distances
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Wood & Churchwell 1989
Finding embedded high mass young stellar objects
T > 100 K
IRAS Point Source Catalog12 + 25 + 60 + 100 µm
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Wood & Churchwell 1989
Palla+ 1991
125 sources fulfill W&C + have HCO+
135 extra sources have HCO+
Many have H2O masers
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Palla+ 1991, 1993Molinari+ 1996, 1998, 2000
125 “high” sources fulfill W&C
135 “low sources have HCO+
“high” sources: •More active
• UCHII, but also younger MP/YSO
•More H2O masers (29%)135 “low sources have HCO+
“low” sources: •less active
• UCHII, but also younger
•fewer H2O (9%) masersTalk by Sergio Molinari
A Sample of Massive Young Stellar Objects
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Very many follow-up studies of Molinari+ sampleExample:
A&A 414, 299 (2004)
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20 y monitoring of ~40 H2O masers with Medicina
Valdettaro+ 2002Brand+ 2003, 2005Felli+ 2007
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Maser monitoring can have big pay-off!!Recently discovered strong outburst of high mass YSO were accompanied (even preempted?) by very strong maser outbursts
Scaled up FUOR accretion episodes?
Factor ~10 luminosity increaseCaratti o Garatti+ 2017
Moscadelli+ 2017
S255
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The value of maser monitoringRecently discovered strong outburst of high mass YSO were accompanied (even preempted?) by very strong maser outbursts
Scaled up FUOR accretion episodes?
Caratti o Garatti+ 2017
Moscadelli+ 2017
Poster 36:: A. Caratti o GarratiPoster 74: B. Stecklum
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ApJ 2017 March
Luminosity surge by a factor ~70 Sudden accretion event? CH3OH 6.7 GHz
H2O 22.2 GHz
Persistent, long-term monitoring
Hartebeesthoek Radio Observ-atory 26m telescope
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Chapter 15:Interstellar Masers
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Water maser research is a significant part of Francesco’s legacy•The Medicina data, taken for themselves, provide valuable targets for
• searches for embedded, active, accreting very young stellar objects
• trigonometric parallax Galactic structure surveys•They also were are the starting point of a large scale program to systematically study high-mass young stellar objects •Future, closely spaced, rapidly reduced variability surveys may point to key objects for the study of episodic accretion events