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20092026
most citedReverberation Mapping Measurements of Black Hole Masses in Six Local Seyfert Galaxies

360 citations · 1.4k across the 41 of their papers we have counts for

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23 papers · 1 filter

astro-ph.SR2026

IPA: Morphology and Kinematics of Molecular Hydrogen Winds in Five Young Protostars across the Mass Spectrum Observed with JWST

Himanshu Tyagi, P. Manoj, Mayank Narang +29

Molecular winds may play a key role in governing angular momentum transport and accretion during the early evolution of protostars. We present the morphology and kinematic properti…

astro-ph.SR2026

Radio Continuum and Water Maser Monitoring of the Outburst in HOPS 373: Free-Free Emission Does Not Respond to the Outburst

John Tobin, Doug Johnstone, Greg Herczeg +5

We present VLA C-band (5~cm) continuum, K-band (1.3~cm) continuum, and water maser (22.235 GHz) monitoring of the protostar HOPS-373. We additionally present the contemporaneous mo…

astro-ph.SR2026

JOYS: A JWST/MIRI survey of the evolution of H winds and jets from low-mass protostars

L. Francis, Ł. Tychoniec, E. F. van Dishoeck +20

Protostellar outflows display wide-angle winds and collimated jets, the magnetocentrifugal launching of which enables accretion onto the protostar. The majority of the outflow mass…

astro-ph.SR2026

Accretion onto the Embedded Protostar L1527 IRS: Insights from JWST NIRSpec and MIRI Observations

W. Blake Drechsler, John J. Tobin, Patrick D. Sheehan +12

Accretion is the primary driver of protostellar evolution, regulating mass assembly and shaping the physical and chemical environments of young stellar objects. Quantifying accreti…

astro-ph.SR2026★ 1 cited

JOYS: JWST MIRI/MRS spectra of the inner 500 au region of the L1527 IRS bipolar outflow

R. Devaraj, E. F. van Dishoeck, T. P. Ray +12

This study characterized the physical and kinematic properties within the innermost 500 au region of the L1527 bipolar outflow, a class 0/I low-mass protostar using JWST MIRI/MRS s…

astro-ph.SR2026★ 1 cited

Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMA

Mayank Narang, Himanshu Tyagi, Nagayoshi Ohashi +37

Understanding the earliest stage of star and planet formation requires detailed observations to address the connection and interplay between the accretion, outflow and disk evoluti…

astro-ph.SR2025★ 1 cited

IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

Dan M. Watson, Mayank Narang, Caeley V. Pittman +41

The earliest stages of star formation are highlighted by complex interactions between accretion, outflow, and radiative processes, which shape the chemical and physical environment…

astro-ph.SR2025

On the protostellar mass-luminosity relation

Lee Hartmann, John J. Tobin, Patrick Sheehan +2

We present a preliminary view of the protostellar mass-luminosity relation using current samples of protostars with dynamical mass estimates. To provide a lower limit to the expect…

astro-ph.SR2025★ 11 cited

HDO ice detected toward an isolated low-mass protostar with JWST

Katerina Slavicinska, Łukasz Tychoniec, María Gabriela Navarro +15

Water is detected in environments representing every stage of star and solar system formation, but its chemical evolution throughout these stages remains poorly constrained. Deuter…

astro-ph.SR2024★ 3 cited

Constraining the Stellar Masses and Origin of the Protostellar VLA 1623 System

Sarah I Sadavoy, Patrick Sheehan, John J. Tobin +6

We present ALMA Band 7 molecular line observations of the protostars within the VLA 1623 system. We map CO (3 - 2) in the circumbinary disk around VLA 1623A and the outflow…

astro-ph.SR2024★ 29 cited

JWST detections of amorphous and crystalline HDO ice toward massive protostars

Katerina Slavicinska, Ewine F. van Dishoeck, Łukasz Tychoniec +19

This work aims to utilize the increased sensitivity and resolution of the JWST to quantify the HDO/HO ratio in ices toward young stellar objects (YSOs) and to determine if th…

astro-ph.SR2023

The CO outflow components ejected by a recent accretion event in B335

Chul-Hwan Kim, Jeong-Eun Lee, Carlos Contreras Peña +4

Protostellar outflows often present a knotty appearance, providing evidence of sporadic accretion in stellar mass growth. To understand the direct relation between mass accretion a…

astro-ph.SR2023★ 1 cited

IPA: Class 0 Protostars Viewed in CO Emission Using JWST

Adam E. Rubinstein, Neal J. Evans, Himanshu Tyagi +24

We investigate the bright CO fundamental emission in the central regions of five protostars in their primary mass assembly phase using new observations from JWST's Near-Infrared Sp…

astro-ph.SR2023

Early Planet Formation in Embedded Disks (eDisk) X: Compact Disks, Extended Infall, and a Fossil Outburst in the Class I Oph IRS43 Binary

Suchitra Narayanan, Jonathan P. Williams, John J. Tobin +17

We present the first results from the Early Planet Formation in Embedded Disks (eDisk) ALMA Large Program toward Oph IRS43, a binary system of solar mass protostars. The 1.3 mm dus…

astro-ph.SR2023

Early Planet Formation in Embedded Disks (eDisk) XII: Accretion streamers, protoplanetary disk, and outflow in the Class I source Oph IRS63

Christian Flores, Nagayoshi Ohashi, John J. Tobin +25

We present ALMA observations of the Class I source Oph IRS63 in the context of the Early Planet Formation in Embedded Disks (eDisk) large program. Our ALMA observations of Oph IRS6…

astro-ph.SR2023★ 1 cited

Discovery of a collimated jet from the low luminosity protostar IRAS 162532429 in a quiescent accretion phase with the JWST

Mayank Narang, Manoj P., Himanshu Tyagi +36

Investigating Protostellar Accretion (IPA) is a JWST Cycle~1 GO program that uses NIRSpec IFU and MIRI MRS to obtain 2.9--28~m spectral cubes of young, deeply embedded protostar…

astro-ph.SR2023★ 53 cited

Investigating Protostellar Accretion-Driven Outflows Across the Mass Spectrum: JWST NIRSpec IFU 3-5~m Spectral Mapping of Five Young Protostars

Samuel Federman, S. Thomas Megeath, Adam E. Rubinstein +35

Investigating Protostellar Accretion is a Cycle 1 JWST program using the NIRSpec+MIRI integral field units to obtain 2.9--28 m spectral cubes of five young protostars with lumin…

astro-ph.SR2021

Which molecule traces what: chemical diagnostics of protostellar sources

Łukasz Tychoniec, Ewine F. van Dishoeck, Merel L. R. van 't Hoff +8

The physical and chemical conditions in Class 0/I protostars are fundamental in unlocking the protostellar accretion process and its impact on planet formation. The aim is to deter…

astro-ph.SR2018★ 92 cited

Methanol and its relation to the water snowline in the disk around the young outbursting star V883 Ori

Merel L. R. van 't Hoff, John J. Tobin, Leon Trapman +5

We report the detection of methanol in the disk around the young outbursting star V883 Ori with the Atacama Large Millimeter/submillimeter Array (ALMA). Four transitions are observ…

astro-ph.SR2017★ 95 cited

The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution

William J. Fischer, S. Thomas Megeath, Elise Furlan +12

The Herschel Orion Protostar Survey obtained well-sampled 1.2 - 870 micron spectral energy distributions (SEDs) of over 300 protostars in the Orion molecular clouds, home to most o…

astro-ph.SR2015★ 99 cited

HOPS 383: An Outbursting Class 0 Protostar in Orion

Emily J. Safron, William J. Fischer, S. Thomas Megeath +11

We report the dramatic mid-infrared brightening between 2004 and 2006 of HOPS 383, a deeply embedded protostar adjacent to NGC 1977 in Orion. By 2008, the source became a factor of…

astro-ph.SR2014★ 38 cited

Characterizing the Youngest Herschel-detected Protostars I. Envelope Structure Revealed by CARMA Dust Continuum Observations

John J. Tobin, Amelia M. Stutz, S. Thomas Megeath +8

We present CARMA 2.9 mm dust continuum emission observations of a sample of 14 Herschel-detected Class 0 protostars in the Orion A and B molecular clouds, drawn from the PACS Brigh…

astro-ph.SR2011★ 53 cited

A Spitzer-IRS Detection of Crystalline Silicates in a Protostellar Envelope

Charles A. Poteet, S. Thomas Megeath, Dan M. Watson +12

We present the Spitzer Space Telescope Infrared Spectrograph spectrum of the Orion A protostar HOPS-68. The mid-infrared spectrum reveals crystalline substructure at 11.1, 16.1, 18…