-
1
-
2
WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs
Published 2025-01-01“…Galaxy interactions can significantly affect the star formation in galaxies, but it remains a challenge to achieve a consensus on the star formation rate (SFR) enhancement in galaxy pairs. …”
Get full text
Article -
3
Massive Clusters and OB Associations as Output of Massive Star Formation in <i>Gaia</i> Era
Published 2025-01-01Subjects: Get full text
Article -
4
Star Formation Law at Sub-kpc Scale in the Elliptical Galaxy Centaurus A as Seen by ALMA
Published 2017-01-01“…The results showed a breakdown in star formation law with a 0.49±0.05 index relating ∑SFR and ∑H2 at 185 pc. …”
Get full text
Article -
5
ALMA Observations of Massive Clouds in the Central Molecular Zone: External-pressure-confined Dense Cores and Salpeter-like Core Mass Functions
Published 2025-01-01Subjects: Get full text
Article -
6
Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF
Published 2025-01-01“…Specifically, we enhanced star formation activity in high-redshift galaxies by either increasing the star formation efficiency up to 100% or adopting a top-heavy initial mass function (IMF). …”
Get full text
Article -
7
Minor-merger-induced Star Formation Rejuvenation in an Elliptical Radio-loud Quasar Host, 3C 59
Published 2025-01-01“…The inferred star formation history of 3C 59 has shown significant star formation rejuvenation within the past 500 Myr, before which it remained rather quiescent for most of the cosmic time. …”
Get full text
Article -
8
An Effect Study of Structural Jets on the Long Gamma-Ray Burst Formation Rate at Low Redshift
Published 2025-01-01Subjects: Get full text
Article -
9
-
10
The Hubble Space Telescope Survey of M31 Satellite Galaxies. IV. Survey Overview and Lifetime Star Formation Histories
Published 2025-01-01“…(iii) ~50% of our M31 satellites show prominent ancient star formation (>12 Gyr ago) followed by delayed quenching (8–10 Gyr ago), which is not commonly observed among the MW satellites. …”
Get full text
Article -
11
Deciphering Gas Dynamics and Star Formation in a z = 1.1 Main-sequence Spiral Galaxy with ALMA and JWST
Published 2025-01-01“…We present a joint analysis of high-resolution CO(2–1) and Paschen- α (Pa α ) emission lines to trace gas dynamics and spatially resolved star formation in ASPECS-LP.3 mm.06, a z = 1.1 main-sequence galaxy. …”
Get full text
Article -
12
Global and Local Infall in the ASHES Sample (GLASHES). I. Pilot Study in G337.541
Published 2025-01-01Subjects: Get full text
Article -
13
Tracking Star-forming Cores as Mass Reservoirs in Clustered and Isolated Regions Using Numerical Passive Tracer Particles
Published 2025-01-01Subjects: “…Star formation…”
Get full text
Article -
14
Discovery of Metal-poor and Distant Pre–Main Sequence Candidates in WLM with JWST
Published 2025-01-01Subjects: “…Star formation…”
Get full text
Article -
15
CEERS: Increasing Scatter along the Star-forming Main Sequence Indicates Early Galaxies Form in Bursts
Published 2025-01-01Subjects: Get full text
Article -
16
A Study of the Star Clusters’ Population in the Giant Molecular Cloud G174+2.5
Published 2025-01-01Subjects: Get full text
Article -
17
A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at z = 4–6
Published 2025-01-01“…We present a stringent measurement of the dust-obscured star formation rate density (SFRD) at z = 4–6 from the ASPIRE JWST Cycle-1 medium and ALMA Cycle-9 large program. …”
Get full text
Article -
18
Minute-cadence Observations of the LAMOST Fields with the TMTS. VI. Physical Parameters of Contact Binaries
Published 2025-01-01Subjects: Get full text
Article -
19
Are Stars Really Ingesting Their Planets? Examining an Alternative Explanation
Published 2025-01-01Subjects: Get full text
Article -
20
Uncovering the Hidden Physical Structures and Protostellar Activities in the Low-metallicity S284-RE Region: Results from ALMA and JWST
Published 2025-01-01Subjects: Get full text
Article