ISSN: 2041-8205

Journal Home

Journal Guideline

Astrophysical Journal Letters Q1 Unclaimed

IOP Publishing Ltd. United Kingdom

Unfortunately this journal has not been claimed yet. For this reason, some information may be unavailable.

Astrophysical Journal Letters is a journal indexed in SJR in Astronomy and Astrophysics and Space and Planetary Science with an H index of 201. It has a price of 2100 €. It has an SJR impact factor of 3,639 and it has a best quartile of Q1. It has an SJR impact factor of 3,639.

Astrophysical Journal Letters focuses its scope in these topics and keywords: disk, observations, protoplanetary, magnetic, dust, tau, stars, matter, hot, flux, ...

Type: Journal

Type of Copyright:

Languages:

Open Access Policy:

Type of publications:

Publication frecuency: -

Categories: Astronomy and Astrophysics (Q1) Space and Planetary Science (Q1)

Price

2100 €

Inmediate OA

NPD

Embargoed OA

0 €

Non OA

Metrics

3,639

SJR Impact factor

201

H Index

730

Total Docs (Last Year)

1751

Total Docs (3 years)

37090

Total Refs

26546

Total Cites (3 years)

1751

Citable Docs (3 years)

14,12

Cites/Doc (2 years)

50,81

Ref/Doc

Other journals with similar parameters

Annual Review of Earth and Planetary Sciences Q1
Astrophysical Journal, Supplement Series Q1
Nature Astronomy Q1
Astronomical Journal Q1
Space Science Reviews Q1

Compare this journals

Aims and Scope

Best articles by citations

A TURBULENCE-DRIVEN MODEL FOR HEATING AND ACCELERATION OF THE FAST WIND IN CORONAL HOLES

A THOUSAND SHADOWS OF ANDROMEDA: ROTATING PLANES OF SATELLITES IN THE MILLENNIUM-II COSMOLOGICAL SIMULATION

A CORRELATION BETWEEN STELLAR ACTIVITY AND THE SURFACE GRAVITY OF HOT JUPITERS

FERMI

X-RAY ACTIVITY PHASED WITH PLANET MOTION IN HD 189733?

THE DETECTION OF ANOMALOUS DUST EMISSION IN THE NEARBY GALAXY NGC 6946

DISCOVERY OF ROTATIONAL BRAKING IN THE MAGNETIC HELIUM-STRONG STAR SIGMA ORIONIS E

PROPAGATION OF THE 2012 MARCH CORONAL MASS EJECTIONS FROM THE SUN TO HELIOPAUSE

DO JETS PRECESS...OR EVEN MOVE AT ALL?

CONSTRAINING EXPLOSION TYPE OF YOUNG SUPERNOVA REMNANTS USING 24 ¬µm EMISSION MORPHOLOGY

DISCOVERY OF STRONG IRON Ka EMITTING COMPTON THICK QUASARS AT

ON THE FORMATION LOCATION OF URANUS AND NEPTUNE AS CONSTRAINED BY DYNAMICAL AND CHEMICAL MODELS OF COMETS

SHOW MORE ARTICLES

NuSTAR

ON THE

THE gamma-RAY EMISSION REGION IN THE FANAROFF-RILEY II RADIO GALAXY 3C 111

EXPANDED VERY LARGE ARRAY OBSERVATIONS OF GALACTIC SUPERNOVA REMNANTS: WIDE-FIELD CONTINUUM AND SPECTRAL-INDEX IMAGING

FINE-SCALE STRUCTURES OF FLUX ROPES TRACKED BY ERUPTING MATERIAL

STOCHASTICITY AND PERSISTENCE OF SOLAR CORONAL MASS EJECTIONS

ROTATION OF THE NGC 1333 IRAS 4A2 PROTOSTELLAR JET

A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND

SHOCKING TAILS IN THE MAJOR MERGER ABELL 2744

HIGH PRECISION K-SHELL PHOTOABSORPTION CROSS SECTIONS FOR ATOMIC OXYGEN: EXPERIMENT AND THEORY

THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A CLOSE SUBSTELLAR COMPANION TO THE YOUNG DEBRIS DISK STAR PZ Tel

PSR J2021+4026 IN THE GAMMA CYGNI REGION: THE FIRST VARIABLE gamma-RAY PULSAR SEEN BY THE

Comments

No comments ... Be the first to comment!

Publication speed *

Review quality *

Edition and editorial team *

Institutional email or ORCID *

* The email or ORCID field is only to validate the authenticity of the comment, the identity will not be public. .

Astrophysical Journal Letters Q1 Unclaimed

2100 €

NPD

0 €

Metrics

3,639

201

730

1751

37090

26546

1751

14,12

50,81

Other journals with similar parameters

Aims and Scope

Best articles by citations

Comments

FAQS

What is the impact factor of Astrophysical Journal Letters?