about
Measuring star formation with resolved observations: the test case of M 33Cool and warm dust emission from M 33 (HerM33es)Cool gas and dust in M 33: Results from the HERschel M 33 Extended Survey (HERM33ES)PACS and SPIRE photometer maps of M 33: First results of the HERschel M 33 Extended Survey (HERM33ES)The JCMT Nearby Galaxies Legacy Survey - VIII. CO data and the LCO(3-2)-LFIR correlation in the SINGS sampleThe Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 Star-forming ClumpThe Green Bank Ammonia Survey: Observations of Hierarchical Dense Gas Structures in Cepheus-L1251The Green Bank Ammonia Survey: Dense Cores under Pressure in Orion AThe Green Bank Ammonia Survey: First Results of NH3 Mapping of the Gould BeltThe JCMT Gould Belt Survey: a first look at Southern Orion A with SCUBA-2The JCMT Gould Belt Survey: evidence for radiative heating and contamination in the W40 complexThe JCMT Gould belt survey: evidence for dust grain evolution in Perseus star-forming clumpsThe JCMT Gould Belt Survey: first results from the SCUBA-2 observations of the Ophiuchus molecular cloud and a virial analysis of its prestellar core populationThe JCMT Gould Belt Survey: evidence for radiative heating in Serpens MWC 297 and its influence on local star formationThe JCMT Gould Belt Survey: a first look at dense cores in Orion BThe JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar discs in L 1495The JCMT Gould Belt Survey: constraints on prestellar core properties in Orion A NorthCloud-scale Molecular Gas Properties in 15 Nearby GalaxiesA Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces. I. Cloud-scale Gas MotionsShock excited molecules in NGC 1266: ULIRG conditions at the center of a bulge-dominated galaxyFull-disc ¹³CO(1–0) mapping across nearby galaxies of the EMPIRE survey and the CO-to-H₂ conversion factorVariations in the star formation efficiency of the dense molecular gas across the disks of star-forming galaxiesALMA multi-line imaging of the nearby starburst NGC 253ALMA reveals the molecular medium fueling the nearest nuclear starburstHierarchical star formation in M33: fundamental properties of the star-forming regionsDense gas in M 33 (HerM33es)A portrait of cold gas in galaxies at 60 pc resolution and a simple method to test hypotheses that link small-scale ISM structure to galaxy-scale processesTowards a new classification of galaxies: principal component analysis of CALIFA circular velocity curvesThe JCMT nearby galaxies legacy survey – X. Environmental effects on the molecular gas and star formation properties of spiral galaxiesDense gas fraction and star-formation efficiency variations in the Antennae galaxiesOptical depth estimates and effective critical densities of dense gas tracers in the inner parts of nearby galaxy discsThe Bolocam Galactic Plane Survey. XIII. Physical properties and mass functions of dense molecular cloud structuresCARMA large area star formation survey: structure and kinematics of dense gas in Serpens mainCARMA large area star formation survey: project overview with analysis of dense gas structure and kinematics in Barnard 1A 50 pc Scale View of Star Formation Efficiency across NGC 628Graph-based interpretation of the molecular interstellar medium segmentationA Catalog of HiClouds in the Large Magellanic CloudCARMA large area star formation survey: observational analysis of filaments in the Serpens south molecular cloudGiant molecular clouds in the early-type galaxy NGC 4526The EDGE–CALIFA survey: the influence of galactic rotation on the molecular depletion time across the Hubble sequence
P50
Q56914276-8e7c68fb-49ad-95bd-96c4-5e1a3f24d73dQ56914885-36A9531D-2A61-4D95-B73A-8EA4E9001F0BQ56915265-3F453656-FAB8-4CAC-9D41-C5B499C653C4Q56915309-01AD79A6-EB69-4975-BB9E-CDD56E5CF0E2Q57088404-61019F76-7B52-4361-8791-013F9AC74DCEQ57757223-C653BB44-0130-4CC5-8BEF-9C156D06E03DQ57757235-4B8E7632-3D47-43F6-8C8A-67F19FB06544Q57757251-BFFEE18A-D8CC-4216-9E9A-65FEF6460D6EQ57757261-F52AD7B4-5528-465C-9D9A-B8680CCF1F80Q57757282-EE7317E8-B39D-481A-A266-CE0B5F1146A8Q57757289-8840E851-41C2-4BF3-8D26-F7B70570098CQ57757293-07F10FE7-4897-4797-BD2A-51A3F1B2A012Q57757333-5FA0A076-6A27-48C9-B68C-715A4ACF0B38Q57757337-6F50213A-22F9-4B39-BE55-61182CA0E209Q58377993-99FE3D0B-1702-4A49-B42F-ED2F57CB83A8Q58501816-0842E18A-6B5C-41C6-9418-72368E69FA05Q58501823-350859EF-F81F-4F81-9659-885D230F6843Q58915789-683F7151-F92B-4961-BDF7-400749B73BF5Q58915791-39B51CA4-C5CE-49F7-AB8F-3F59E2DDF2FEQ58915915-252ECFE5-B9F8-478F-ABC3-65B5C36A8FC4Q58921973-5DB45BBF-E06F-413E-BFB0-045B8D3C9C29Q58922061-98F18049-0017-4A24-B270-FF7FD00825F7Q58922076-579CA4D4-547C-488A-B1B8-A806CA6E2714Q58922078-A5C13F98-6D6C-4842-8190-FA49BF036C59Q59111318-CA3D7064-25AB-4FAF-B700-D3DE0CC398AAQ59751398-B329CA11-E2A5-452A-8038-ECD789AE032FQ59887147-0312D109-423E-4C44-B609-B35230859B97Q59906882-2AA44F15-0D39-47DB-B34A-25030AA8637CQ59923980-E656A4F1-912B-4B81-8C2F-7DB9309B584FQ59938933-2E0E64DB-28BE-4EBC-BBD9-65F3EE8164BDQ59939661-4C38957D-2BE4-466E-9697-6F71086746DCQ59959433-6998F0BB-CF78-4439-88E8-27FBEF3EFE20Q59974223-FCFE0507-FF6F-4F8F-BD0C-8281832D5B82Q59974229-D13CDADE-6625-4EE3-B389-4AE2E6871F3AQ60015655-002F9582-AFD5-460D-A2E9-6D5A3686E549Q60018446-2BBCFC2F-D840-4127-80DD-66C5CF21DB02Q60504250-E17CEA90-BA10-427A-95E4-E7F42CBFA2D9Q60708165-D6195768-3966-43B2-9843-D82958C0E5FFQ62620077-2A3EF33B-4DBF-4902-91CE-2D69C62AF831Q62623041-11F07066-DC7A-40EE-AFA5-BF4E55E5A0DF
P50
description
researcher, ORCID id # 0000-0002-5204-2259
@en
wetenschapper
@nl
name
Erik Rosolowsky
@ast
Erik Rosolowsky
@en
Erik Rosolowsky
@es
Erik Rosolowsky
@nl
type
label
Erik Rosolowsky
@ast
Erik Rosolowsky
@en
Erik Rosolowsky
@es
Erik Rosolowsky
@nl
prefLabel
Erik Rosolowsky
@ast
Erik Rosolowsky
@en
Erik Rosolowsky
@es
Erik Rosolowsky
@nl
P106
P31
P496
0000-0002-5204-2259