The distance of M33 and the stellar population in its outskirts
We present deep V,I photometry of two $9.4' x 9.4' field in the outer regions of the M33 galaxy. We obtain a robust detection of the luminosity of the Red Giant Branch Tip (I{TRGB}=20.72 +- 0.08) from which we derived a new estimate of the distance ...
Bellazzini +54 more
core +1 more source
Obscured Asymptotic Giant Branch stars in the Magellanic Clouds III. New IRAS counterparts [PDF]
J. Th. van Loon +5 more
openalex +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
FEAST: Probing the Stellar Population of the Starburst Dwarf Galaxy NGC 4449 with JWST/NIRCam
We present new JWST/NIRCam observations of the starburst irregular galaxy NGC 4449, obtained in Cycle 1 as part of the Feedback in Emerging extrAgalactic Star clusTers program, which we use to investigate its resolved stellar populations and their ...
Matteo Correnti +24 more
doaj +1 more source
Submillimeter and infrared studies of mass lost by asymptotic giant branch stars [PDF]
Kenneth H. Young
openalex +1 more source
Carbon Stars as Standard Candles: An Empirical Test for the Reddening, Metallicity, and Age Sensitivity of the J-region Asymptotic Giant Branch (JAGB) Method [PDF]
Abigail J. Lee
openalex +1 more source
Sodium production in asymptotic giant branch stars
[condensed] A new scenario is presented for the production of Na23 in asymptotic giant branch (AGB) stars. The scenario takes advantage of the periodic third dredge-up episodes characterizing those stars, which mix primary C12 from their intershell layers to their surface. Two successive interpulse/pulse/dredge-up sequences are then required to produce
openaire +2 more sources
Radiation-Pressure Ejection of Planetary Nebulae in Asymptotic-Giant-Branch Stars [PDF]
A. V. Sweigart
openalex +1 more source
Observations of Molecular CN toward S-type Asymptotic Giant Branch Stars
S-type asymptotic giant branch (AGB) stars are defined by their carbon-to-oxygen (C/O) ratio approaching unity. However, observations of circumstellar molecules in these stars are limited and challenging.
Yanan Feng +11 more
doaj +1 more source
Dust Structure Around Asymptotic Giant Branch Stars – CORRIGENDUM [PDF]
Devendra Raj Upadhyay +3 more
openalex +1 more source

